The galaxy presents an overall elliptical morphology, though not perfectly round, appearing somewhat intermediate in ellipticity. The light distribution is centrally concentrated with a bright core, suggesting a significant bulge component. Faint, diffuse extensions are visible, indicating a possible disk component or tidal features. A slight asymmetry in the outer regions is seen, suggestive of possible minor interactions or disturbances. The color appears generally blue-white, implying the presence of relatively young, hot stars, although the core region seems somewhat less blue, which could be from old stars, or dust. The galaxy is neither obviously undergoing a major merger nor is it completely undisturbed, which would suggest a recent minor interaction or internal dynamics causing subtle disruptions to its overall structure.
