The galaxy appears to be a relatively smooth system. Its morphology is largely elliptical, showing a centrally concentrated bulge. The light profile gradually decreases from the core outwards. There is a slight elongation along one axis, which implies the galaxy is not perfectly spherical, trending towards a cigar shape. No distinct spiral arms or prominent dust lanes are readily apparent in the image. There is no obvious major interaction or merger activity. The color profile appears rather uniform throughout the galaxy. The light suggests older stellar populations dominate. Any star forming regions that may exist are not prominent.
