The galaxy presents as a flattened, elliptical-like structure. It exhibits a central bulge that appears luminous and concentrated, with a smooth transition from the bright core to the outer regions. The overall color suggests a combination of stellar populations, with a possible prevalence of older, redder stars in the bulge, and a slightly bluer, more diffuse halo indicative of younger stars or regions of ongoing star formation. There may be some evidence of a faint, extended disk, though it is not prominently defined. The morphology is largely undisturbed, showing no strong signs of major mergers or significant tidal interactions. Faint spiral arm features cannot be ruled out.
