The galaxy presents an elliptical morphology, appearing largely smooth and centralized. The light distribution indicates a bright central bulge that fades gradually towards the outer regions. The lack of distinct spiral arms or prominent dust lanes suggests a relatively evolved system. Color gradients are subtle, with a tendency towards redder hues in the central region, potentially indicating a population of older stars, and bluer tints in the outer fringes of the disk due to a younger population of stars. There is no indication of any major mergers or tidal disturbances in the vicinity. The overall impression is that of a well-formed, quiescent galaxy with minimal ongoing star formation.