The galaxy presents as a relatively smooth, centrally concentrated object with a generally elliptical morphology, appearing close to round. The core exhibits a bright, diffuse glow. The surrounding halo exhibits a bluer tint compared to the central region, suggesting the presence of younger stellar populations in the outer regions, though the smooth texture of the galaxy overall hints at a largely quiescent stellar formation rate. There is no visible evidence of strong spiral arm structure, bar structure, or major tidal disturbances, indicating the galaxy has likely not undergone a recent major merger event. Minimal dust lanes or patches are visible within the galaxy. The object exhibits some color variation, which indicates some ongoing star formation. Overall, the galaxy appears to be a fairly typical, relaxed system with a dominant smooth component.
