The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core region exhibits a bright, yellowish-white color, suggesting a population of older stars. The isophotes appear generally round with only slight deviations. There is a faint, diffuse halo surrounding the central region, extending outwards. The color of the halo appears slightly bluer than the core, which may be due to a small amount of younger stars. There is no apparent dust lane visible. The overall appearance indicates a galaxy that is not currently undergoing significant star formation and shows no signs of a major merger.
