The galaxy presents as a centrally concentrated, elliptical-like object with a smooth light distribution. The core appears as a bright, yellowish-white region. The overall color suggests a population of older stars, with a lesser presence of blue light indicative of younger stars. There is very little evidence of spiral arms or disk structure. The outer regions exhibit a faint, diffuse halo, gradually fading into the background sky. There are no visible signs of recent major mergers or significant tidal disturbances, such as streams or shells. The galaxy exhibits a high degree of rotational symmetry.
