The galaxy presents as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge, visually dominating the galaxy's overall luminosity. The light from the galaxy appears yellowish-white, suggesting a population of older stars. No distinct spiral arm structures or significant dust lanes are visible. The outer regions fade gradually, indicating a diffuse halo surrounding the central bulge. The galaxy's shape is more elongated than circular, leaning towards an "in between" or possibly even a "cigar shaped" form. There is no apparent evidence of any major ongoing merger activity or significant tidal disturbances, suggesting the galaxy is relatively undisturbed. Given its smooth morphology and color, the galaxy likely exhibits a low star formation rate.
