The galaxy appears to be an elliptical galaxy, possibly of type E4-E6. It presents a generally smooth profile, with the light gradually decreasing from the center. The galaxy exhibits a notable elongation. There is a suggestion of a disk structure. No spiral arms are readily apparent. The central bulge is bright and concentrated. The lack of distinct features suggests a relatively old stellar population, and a low star formation rate. There seems to be a minor gravitational disturbance taking place.
