The galaxy presents as a flattened, elliptical form with a bright, concentrated central bulge. The overall color profile suggests an older stellar population, with a yellowish-orange hue dominating the central region. Fainter, bluer regions extend along the major axis, suggestive of some ongoing, albeit reduced, star formation within a disk-like component. The galaxy exhibits a relatively smooth structure with no obvious signs of major mergers or significant tidal disturbances. It has a slight elongation, appearing somewhat cigar-shaped when observed at its given inclination.
