The galaxy presents as a relatively compact, elliptical-like structure. It exhibits a smooth, centralized concentration of light, with a distinct lack of spiral arm features or significant disk-like morphology. The galaxy displays a diffuse, moderately bright halo surrounding a denser, brighter core. There is no obvious presence of dust lanes or prominent star-forming regions. The overall color appears somewhat redder, indicative of a population of older stars and lower levels of recent star formation. The light profile suggests a relatively relaxed system, possibly in a later stage of its evolutionary process. Subtle hints of a possible tidal tail or minor disturbances are present, suggesting a past interaction or accretion event. The object does not appear to be actively merging.
