This galaxy appears to be a relatively small, elliptical or lenticular type. Its central region displays a high surface brightness, suggesting a dense concentration of stars. The core is roughly circular with a mostly homogenous bright white/blue color. There's some slight evidence of minor disturbances or tidal features, notably an extension in the northwestern quadrant and a bit in the southern part of the galaxy. These subtle asymmetries could be indicative of a past minor merger or interaction. The galaxy exhibits a faint, diffuse halo extending outwards with light dropoff, contributing to its overall size. The object's color indices suggest a significant population of older stars, although a component of younger, bluer stars may be present in the core. Overall, the galaxy appears to be in a relatively settled state with potential signs of past gravitational interactions.
