The galaxy presents as a relatively smooth, elliptical-like structure. Its overall color appears reddish, indicating a population of older stars and a relatively low rate of current star formation. There is very little discernible disk structure. The galaxy displays a high degree of central concentration, with the light intensity decreasing smoothly towards the outer edges. There is slight visual evidence of minor disturbances, possibly indicating past or ongoing minor interactions with smaller galaxies or the accretion of intergalactic gas. It shows a generally round shape.
