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We consider non-commutating Simpson-Visser spacetime and study thesuperradiance phenomena and the shadow cast by the back hole associated withthis modified spacetime. We extensively study the different aspects of theblack hole associated with the metric endowed with the corrections linked withnon-commutative properties of spacetime. We study the superradiance effect,deviation of shape, size of the ergosphere, and the shadow of black hole inthis extended situation and look into their variation taking different valuesSimpson-Visser parameter $\ell$ and non-commutative parameter $b$. We have madean attempt to constrain the parameter $\ell$ using the data available from theEHT collaboration for $M87^*$ black hole. Our study reveals that black holesare associated with non-commutative Simpson-Visser spacetime may be a suitablecandidate for an astrophysical black hole.

Superradiance scattering off rotating Simpson-Visser black hole and its shadow in the non-commutative setting