The galaxy presents as a single, relatively smooth object. Its overall morphology is elliptical, exhibiting a concentrated central bulge. The light distribution appears even and symmetrical, with no readily discernible spiral arm structure. Color gradients suggest a centrally concentrated stellar population that is evolved and redder. The overall color suggests minimal ongoing star formation activity. There is no obvious evidence of tidal tails or other morphological disturbances. The galaxy appears to be a relaxed system.
