The galaxy presents as a relatively smooth, centrally concentrated object. It is roughly elliptical in shape, but has more of a disk like apperance, with the ratio of the major to minor axes being approximately 2:1. There is little evidence of spiral arms or dust lanes. The color is moderately red, suggesting an older stellar population and reduced star formation rate. While the galaxy's light is primarily concentrated in the central bulge, there may be some structure surrounding the galaxy, potentially consisting of fainter and older stars. There is no sign of it undergoing a major merger or significant tidal disruption, but it could be experiencing minor interactions.
