The galaxy presents as a luminous, centrally concentrated object. It exhibits a flattened, elliptical morphology, appearing more oblate than perfectly spherical. The central region displays a high surface brightness, suggesting a dense concentration of stars. The light is generally smooth, with a subtle color gradient from the core outwards, becoming slightly bluer toward the periphery. There is no obvious presence of spiral arms or significant dust lanes. Minor asymmetries may be present, but generally, the structure appears largely undisturbed, suggesting a galaxy that has undergone limited recent mergers or interactions.
