The galaxy appears to be a relatively smooth, elliptical-type galaxy, exhibiting a generally spheroidal morphology. There's a concentrated, bright central bulge that transitions to a more diffuse halo. The light distribution suggests an older stellar population.

Color gradients are subtle, with the central bulge appearing somewhat yellower and the outer regions exhibiting a bluer hue. There is a noticeable lack of distinct spiral arm structure or prominent dust lanes. The overall symmetry suggests a relaxed system with minimal signs of recent mergers or tidal disturbances, although a faint asymmetry may be present.
