  We study the behavior of the noncommutative radiating Schwarzschild black
hole in the Finslerian spacetime. The investigation shows that black hole
possesses either (i) two horizons, or (ii) a single horizon, or (iii) no
horizon corresponding to a minimal mass. We obtain that the minimal mass
significantly changes with the Finslerian parameter, keeping minimal horizon
remain unchanged. It turns out that under Finslerian spacetime, the maximum
temperature before cooling down to absolute zero varies with Finslerian
parameter. We then study the stability of the black hole by analyzing the
specific heat and free energy. The energy conditions, their violation limit
also scrutinized. Our findings suggest a stable black hole remnant, whose mass
and size are uniquely determined in terms of the Finslerian parameter
$\overline{Ric}$ and noncommutative parameter $\theta$. The physical relevance
of these results are discussed in a brief.
