The galaxy presents a generally smooth, elliptical morphology. Its color profile suggests a higher concentration of older stellar populations, emitting primarily in the redder bands. The core region exhibits a bright, concentrated intensity, transitioning gradually to a less luminous outer halo. There is no strong evidence of distinct spiral arm structure, bar features, or significant dust lanes. The overall shape appears relatively round and undisturbed, although there might be a very subtle asymmetry present. There is no readily apparent evidence of an ongoing major merger. Some minor disturbances or faint tidal features might be present in the extended halo, but they are difficult to discern with certainty. 
