The galaxy presents as a luminous object with an elliptical morphology. Its core is a bright, concentrated region, suggesting a high density of stars and possibly a supermassive black hole actively accreting material. The intensity of light decreases gradually from the center outwards, indicating a smooth distribution of stellar populations, with older stars likely dominating the overall light profile. There may be a faint disk or ring of material surrounding the galaxy, though it is difficult to see. The overall color of the galaxy leans towards the redder end of the spectrum, signifying an older stellar population with fewer young, hot stars. The galaxy appears relatively undisturbed, with no obvious signs of recent major mergers or tidal interactions that could disrupt its overall structure. There may be evidence of a minor companion galaxy, or a faint tidal stream. Overall, it is a relatively massive galaxy, based on its luminosity and extent. The estimated star formation rate appears relatively low. 
