The galaxy presents as a relatively smooth, centrally concentrated object. The light profile appears to be dominated by a bulge component, with little or no visible disk structure. Color gradients are subtle, but suggest a central region that is slightly redder in comparison to the outer regions, which exhibit a bluer hue. This may be caused by an older stellar population in the center and younger stellar populations in the outskirts. The overall shape appears close to circular with no apparent signs of any major mergers or disturbances.
