The galaxy presents a generally smooth appearance with some indication of features. The central region exhibits a bright core that fades outwards into a more diffuse halo. It appears to be more elongated than circular in shape, with hints of a disk-like structure. There seems to be some degree of asymmetry or disturbance present, possibly a minor interaction or the early stages of a merger event. A small tidal tail or bridge like structure appears to be forming, extending outward from the main body of the galaxy. The colour distribution across the galaxy suggests a mix of stellar populations. The core appears yellower, indicating older stars, while bluer regions are visible which may be associated with regions of active star formation.
