The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge, brighter and yellower in color. The outer regions appear more diffuse, with a subtle color gradient suggesting bluer stellar populations towards the periphery, though this feature is subtle. There is a lack of defined spiral arm structure or prominent dust lanes. Its shape appears generally round. No significant tidal features or evidence of a major merger event are readily apparent, though there are subtle disturbances in the outer halo region. Overall, the galaxy appears relatively quiescent, with a low rate of star formation.
