  We consider non-commutating Simpson-Visser spacetime and study the
superradiance phenomena and the shadow cast by the back hole associated with
this modified spacetime. We extensively study the different aspects of the
black hole associated with the metric endowed with the corrections linked with
non-commutative properties of spacetime. We study the superradiance effect,
deviation of shape, size of the ergosphere, and the shadow of black hole in
this extended situation and look into their variation taking different values
Simpson-Visser parameter $\ell$ and non-commutative parameter $b$. We have made
an attempt to constrain the parameter $\ell$ using the data available from the
EHT collaboration for $M87^*$ black hole. Our study reveals that black holes
are associated with non-commutative Simpson-Visser spacetime may be a suitable
candidate for an astrophysical black hole.
