  In this paper, the shadow casted by the rotating black hole inspired by
noncommutative geometry is investigated. In addition to the dimensionless spin
parameter $a/M_{0}$ with $M_{0}$ black hole mass and inclination angle $i$, the
dimensionless noncommutative parameter $\sqrt{\vartheta}/M_{0}$ is also found
to affect the shape of the black hole shadow. The result shows that the size of
the shadow slightly decreases with the parameter $\sqrt{\vartheta}/M_{0}$,
while the distortion increases with it. Compared to the Kerr black hole, the
parameter $\sqrt{\vartheta}/M_{0}$ increases the deformation of the shadow.
This may offer a way to distinguish noncommutative geometry inspired black hole
from Kerr one via astronomical instruments in the near future.
