The galaxy presents as a largely smooth and centrally concentrated object. It exhibits a yellow-white hue, suggesting a population of older stars and a relatively low rate of ongoing star formation. The overall morphology appears elliptical or lenticular, with a high degree of circularity. There is no visible evidence of spiral arms or a prominent disk structure. The galaxy appears relatively undisturbed, showing no signs of major mergers or significant tidal interactions. There may be a faint, diffuse halo surrounding the central region, but its extent is difficult to ascertain from this image. The object displays a moderate luminosity.
