  We study the shadow and energy emission rate of a spherically symmetric
non-commutative black hole in Rastall gravity. Depending on the model
parameters, the non-commutative black hole can reduce to the Schwarzschild
black hole. Since the non-vanishing non-commutative parameter affects the
formation of event horizon, the visibility of the resulting shadow depends on
the non-commutative parameter in Rastall gravity. The obtained sectional
shadows respect the unstable circular orbit condition, which is crucial for
physical validity of the black hole image model.
