The galaxy presents an elliptical morphology with a smooth, concentrated central bulge that appears yellowish. This likely indicates an older stellar population dominating the core. The outer regions display a slightly flattened shape, with a faint disk component appearing greenish. This green tint may be indicative of a small amount of ongoing star formation. There is some indication of a minor asymmetry to the galaxy, possibly due to a minor gravitational interaction or internal dynamics. No distinct tidal tails or signs of a major merger are apparent. Overall, the galaxy presents a well-defined structure with subtle features suggesting limited recent activity.
