The galaxy presents as a concentrated, elliptical-appearing structure with a smooth light distribution. Its core is luminous, with a diffuse halo fading into the background. There are hints of a more elongated morphology, though its classification tends towards a smooth, not perfectly round shape. There is no strong evidence of significant spiral arm structure or prominent dust lanes. The galaxy does not seem to be strongly interacting with any large companions, although some morphological disturbance can be detected, possibly reflecting a recent minor merger event. The general color suggests that it is a massive galaxy with older stellar populations and relatively low star formation activity.
