The galaxy exhibits a generally smooth morphology, appearing elliptical in shape with a high degree of roundness. It possesses a bright, concentrated core which fades into a diffuse halo. The overall color is slightly reddish, implying a population of older stars and a low star formation rate. There is no apparent presence of spiral arms or significant dust lanes. Minor disturbances cannot be definitively ruled out, but there is no clear visual evidence of a major ongoing merger or tidal interaction. The galaxy presents a mature, evolved appearance.
