We review a recent proposal for a quantum black hole as a certain large N matrix quantum mechanics. In this model, black hole horizon in general relativity is replaced by a fuzzy geometry. The model has past a number of tests: i) the macroscopic mass-size-shape-angular momentum relation for Schwarzschild and Kerr black hole is reproduced. ii) Berkenstein-Hawking entropy is reproduced from a microstates counting. iii) The Hawking radiation is described consistently in terms of quantum mechanical tunneling of the fuzzy sphere via the nucleation of a fuzzy monopole on the horizon. Further directions will be discussed.