No, it is not possible in theory. The short reasoning is: we model the motion of a test particle under gravity via timelike geodesic motion in general relativity, "faster than the speed of light" means a spacelike tangent vector, and geodesics preserve their timelike vs. spacelike vs. lightlike nature.
A more physical argument uses conservation of energy in the rest frame of each black hole individually. For simplicity of the argument, I'll assume the black holes are very far apart, so we can consider them separately and meaningfully discuss the speed of the test mass in a special-relativistic manner between the slingshots. The way a slingshot maneuver works is that the test mass' initial and final speeds are the same in the rest frame of the black hole due to conservation of energy (this holds exactly in GR if one models the black hole as Schwarzschild or Kerr in its rest frame), but its velocity gets redirected. If this velocity is redirected in such a way that it's more aligned with the motion of the black hole in your lab frame, then in the lab frame its speed has increased. See the still taken from a gif of an example scenario on the gravity assist Wikipedia article below:

The "planet" here would be our black hole and the "sun frame" would be our lab frame, but the essentials of the dynamics are the same. The blue trajectory is that of the test mass, while the black trajectory is that of the black hole. To be quantitative: if $v$ is both the initial (nonrelativistic) speed of the test mass in the black hole's frame and the speed of the black hole in the lab frame, then in the pictured scenario the test mass' speed increases from $\sqrt{2} v$ to $2v$ in the lab frame.
So, what about passing the speed of light? The point is that, in each maneuver, the test mass' initial speed is the same as its final speed in the rest frame of the appropriate black hole, so its speed in the lab frame after each maneuver is always some Lorentz transformation of a speed less than $c$. Since it was going less than the speed of light in the black hole frame, it will still be going less than the speed of light in the lab frame-- this is a constraint set by the relativistic velocity-addition formula.
As a demonstration: in the example above, if the speed $v$ were relativistic, the initial and final speeds $u_i,\, u_f$ of the test mass in the lab from would be (using units with $c=1$)
$$u_i = v\sqrt{2-v^2}, \;\; u_f = \frac{2v}{1+v^2}.$$
Notice $u_f < 1$. The test mass need not ever stop accelerating, as it can always change its direction, but it will eventually be unable to meaningfully gain speed due to the above constraint of the addition formula.