What you propose is theoretically but not practically possible. Or rather, we can not really tell the difference. Shining a bunch of lasers at a common point is a good example of a rather complicated scattering experiment. You're creating huge numbers of photons which all have the same energy and bouncing them off each other.
In quantum physics, we don't actually get to watch the details of the scattering; that would interfere with the experiment. Instead all we can do is count the frequency of fixed inputs creating various outputs, and compare these frequencies to probabilities we compute using the rules of quantum physics. In quantum physics, this probability is the norm of a complex number, called the amplitude. We can compute the amplitude for a particular input -> output by adding up amplitudes for every possible way the inputs might turn into the outputs, summing over all possible histories.
So, if you can imagine black holes being formed when you concentrate enough photons in a small area and then being unformed by quantum leakage like Hawking radiation, then you ought to include an amplitude for this in the sum over histories.
One of the big questions in theoretical physics right now is: "Exactly precisely what number should this 'a black hole appears and then disappears' amplitude be?" We really don't know how to compute it precisely.
But we can estimate its order of magnitude in various ways.
For example: A photon in a blue laser has a wavelength of about $\lambda =450$ nm, equivalently an energy $E = \hbar \nu = \hbar c/\lambda$ of around $2$ eV $\sim 10^{-19}$ Joules. We know gravity is pretty weak in distance scales near $\lambda$ on our planet. Newton's constant $G$ is very small; equivalently the Planck mass $M_P \sim 1/\sqrt{G} \sim 10^{30}$ eV is huge. We can try thinking of photons forming a black hole in terms of photons exchanging gravitons.
The methods of quantum field theory tells us that if two photons collide/approach closely the effective coupling constant for a 2-photons and 1 graviton is going to vary with the energy $E$ roughly as $E/m_P$. So for photons in a blue laser, we're going to see everything we calculate multiplied by powers of $10^{-30}$. This makes the contribution of the black hole to the scattering amplitude very small, which makes it all but impossible to measure with current technology.