The galaxy presents a roughly circular morphology, with an overall smooth appearance. The light distribution appears concentrated, with a brighter core region surrounded by a more diffuse halo. There is evidence of a possible ongoing merger or tidal interaction. The galaxy's light is predominantly yellowish in the core with an extension exhibiting a slightly bluer tint, indicating differential stellar populations or dust content within the galaxy. Observed morphology indicates a possible smooth elliptical galaxy in the process of merging with a smaller, bluer object, or potentially a galaxy experiencing an interaction.
