The galaxy presents an elliptical morphology, though it is not perfectly spherical. It displays a smooth, centrally concentrated luminosity profile, with a bright, yellowish core indicative of an older stellar population. The outer regions exhibit a bluer hue, suggesting the presence of younger stars or some ongoing star formation, although at a relatively low rate. There is a subtle hint of disturbance or asymmetry in the outer halo, possibly indicating a past minor merger event or tidal interaction. The overall structure appears relatively relaxed, and the galaxy does not show any signs of a major ongoing merger.
