  We investigate the behavior of a radiating Schwarzschild black hole toy-model
in a 2D noncommutative spacetime. It is shown that coordinate noncommutativity
leads to: i) the existence of a minimal non-zero mass to which black hole can
shrink; ii) a finite maximum temperature that the black hole can reach before
cooling down to absolute zero; iii) the absence of any curvature singularity.
The proposed scenario offers a possible solution to conventional difficulties
when describing terminal phase of black hole evaporation.
