The galaxy presents a largely smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, with light intensity decreasing gradually outward from a bright, yellowish core. There is little to no evidence of spiral arm structure, dust lanes, or significant features suggestive of recent or ongoing major mergers. The galaxy appears relatively undisturbed, with a generally round shape, although there is a very slight deviation from perfect circularity. The outer regions display a faint, diffuse halo. The overall color suggests a population of older stars and a relatively low rate of current star formation.
