The galaxy appears to be a relatively compact system with a smooth, elliptical morphology. It exhibits a centrally concentrated brightness profile, suggesting a significant bulge component. There is little evidence of spiral arms or a well-defined disk structure. The overall color of the galaxy is somewhat blue, indicating the presence of at least some young, hot stars, however is not strongly indicative of ongoing star formation. The galaxy appears relatively undisturbed, without obvious signs of tidal interactions or major mergers. Based on the ellipticity, the galaxy appears close to round. Faint disturbances may be present, but are very minor.
