The galaxy presents as a luminous, centrally concentrated object. Its morphology appears largely smooth, with a high degree of central symmetry. The overall shape is elliptical, but not perfectly round, displaying a slightly elongated form. There is a suggestion of a disk but this is not clearly expressed in the image. The color appears to be a yellow-white hue, suggestive of an older stellar population. There is little evidence of active star formation regions within the galaxy itself. The relative isolation and lack of obvious tidal features indicates it is unlikely to be undergoing a major merging event, though some indications suggest minor disturbances may be present.
