The galaxy appears as an elliptical or lenticular type system, exhibiting a relatively smooth and concentrated light profile. It appears to be moderately inclined along the plane of sight. A bright central bulge is apparent, with a gradual decrease in luminosity towards the outer regions. The overall color index suggests a population of older stars, with a hint of ongoing star formation. There are no obvious signs of spiral arms or prominent dust lanes, with the system presenting a mostly homogenous structure. The overall shape appears somewhat elongated, with a ratio of major to minor axes approximately 3:1. There are no signs of any major mergers or significant tidal disturbances.
