  We study the effect of baryonic matter and apparent dark matter on black hole
shadow in Verlinde's Emergent Gravity. To do so, we consider different baryonic
mass profiles and an optically-thin disk region described by a gas in a radial
free fall around the black hole. Assuming that most of the baryonic matter in
the galaxy is located near the galactic center surrounding a supermassive black
hole, we use two models of power law mass profile for the baryonic matter to
study the effect of apparent dark matter on the shadow and the corresponding
intensity. We find that the effect of the surrounding matter on the shadow size
using observational values is small, however, it becomes significant when the
surrounding baryonic matter increases. To this end, we show that the effect of
simple power law function in the limit of constant baryonic mass in Verlinde's
theory implies an apparent dark matter effect which is similar to the standard
gravity having an isothermal dark matter profile. We also find the intensity of
the electromagnetic flux radiation depending on the surrounding mass.
