The galaxy appears to be a relatively smooth, elliptical or lenticular type. There's a concentrated central bulge exhibiting a yellowish hue, suggestive of an older stellar population. Surrounding the core is a more diffuse halo with subtle color variations. There are some minor disturbances in the shape, but generally no strong tidal features or indications of a major ongoing merger. There appears to be a subtle disk component as well, which suggests there may be some recent star formation, and that it is not only composed of older stars. Overall, the galaxy exhibits characteristics consistent with a significant mass and intermediate star formation rate.
