The galaxy appears to be a relatively smooth, elliptical-like structure with a concentrated central bulge. The overall color is yellowish-red, suggesting an older stellar population and limited ongoing star formation. There is a slight elongation, giving it an overall "in-between" rounded shape. No distinct spiral arms or disk features are readily apparent. There is no clear sign of major disturbances or mergers in its immediate structure, although there are indications of minor irregularities or diffuse extensions around the central core, which could be signs of past interactions.
