The galaxy presents a generally elliptical morphology, although some irregularities can be observed. The central bulge exhibits a high surface brightness and a yellowish-white hue, indicating a population of older stars. Proceeding outward from the core, the galaxy displays a decreasing surface brightness gradient, with a transition to a bluer color, suggestive of ongoing star formation in the outer regions. Faint, diffuse arms or tidal features can be observed extending from the main body of the galaxy, particularly along the edges, which might be indicative of past or ongoing gravitational interactions with another galaxy. Overall, it appears to be a relatively massive galaxy with a mix of old and young stellar populations, possibly undergoing minor disturbances.
