The galaxy presents a generally smooth, elliptical morphology with a bright, concentrated central bulge. The overall color suggests a population of older stars, with a subtle hint of bluer regions indicating potential ongoing, albeit low-level, star formation. The galaxy appears relatively isolated, with no obvious signs of a major merger event, though there may be minor disturbances in the outer regions suggesting a past interaction or accretion event. The overall shape appears to be somewhere between round and slightly elongated.
