The galaxy presents as a relatively smooth, yet somewhat disturbed morphology. It appears elliptical in shape, with a slight elongation. The light distribution suggests a centrally concentrated bulge. There are no discernible spiral arms or prominent dust lanes, however there is some subtle evidence of possible minor tidal distortions. A subtle hint of faint, extended stellar material surrounding the galaxy indicates a more complex interaction history that may not be readily apparent at the current observation depth and resolution. The color profile indicates the presence of intermediate-age stellar populations. Star formation appears moderate, with no highly active regions visible, corresponding with a smooth, featureless disk or bulge. The system does not display characteristics of a major merger, however the morphology suggests some form of interaction has likely occurred.
