The galaxy presents as a somewhat rounded, centrally concentrated object. It appears to possess a smooth, rather featureless morphology. The light distribution suggests a centrally dominant bulge component with a possible faint disk. There is a possible minor disturbance in the galaxy, which may be indicative of a past minor interaction. The light profile appears to be relatively uniform in color, trending toward redder hues in the center. It does not exhibit prominent spiral arms or well-defined dust lanes.
