The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge that appears yellow/orange in color. The morphology is suggestive of an early-type galaxy with a high degree of sphericity. While the galaxy appears mostly smooth, there are suggestions of subtle asymmetries in its outer regions, with hints of a faint, diffuse halo. There is little evidence of distinct spiral arm structure or significant dust lanes, and the overall color profile indicates a population of older stars with suppressed star formation. There is no obvious indication of a major ongoing merger, though subtle disturbances cannot be ruled out. 
