The galaxy presents a generally smooth, elliptical morphology with a concentrated central bulge. A slight elongation is discernible, but the overall shape is predominantly round. The light distribution appears relatively uniform across the galaxy, indicating a lack of significant spiral arm structure or prominent dust lanes. The color gradient suggests a redder core transitioning to slightly bluer outer regions, which could indicate older stellar populations concentrated in the center with some younger star formation activity in the periphery, albeit at a low rate. No signs of major disturbances or merging activity are apparent within the visible structure of the galaxy.
