The galaxy appears to be a relatively smooth, elliptical-type galaxy. It exhibits a concentrated central bulge, with light gradually decreasing outwards. The color is predominantly yellowish-orange. There is no discernible spiral arm structure. The galaxy appears somewhat rounded in shape, although there is a slight elongation or asymmetry. Based on the data available, there is no apparent major merger, or obvious tidal distortion. The galaxy appears to have a centrally concentrated light distribution, indicative of an older stellar population.
