The galaxy presents as a relatively smooth, elliptical object. The light distribution is concentrated towards the center, suggesting a dominant bulge component. There is a noticeable lack of distinct spiral arm structures or prominent dust lanes. The color appears generally redder than typical spiral galaxies, possibly indicative of an older stellar population and lower star formation rate. There may be some minor disturbances or possible merging activity, but the overall structure suggests it is not currently undergoing a major interaction. The roundness of the galaxy is high.
