The galaxy presents as a relatively smooth, centrally concentrated object. Its light profile suggests a dominant spheroid component, with a fuzzy appearance, that gradually fades with increasing radius. The central region exhibits a bright, almost unresolved core. The galaxy's overall shape tends towards rounded, displaying only a slight deviation from perfect circularity. There is no evidence of strong spiral arm structure or a prominent disk component. No significant tidal features, major disturbances, or indications of ongoing or recent major merger activity are discernible in the image. Color gradients are subtle, with a slightly bluer hue in the outer regions suggesting some ongoing, albeit subdued, star formation.
