The galaxy presents as a relatively smooth, elliptical-like structure. It appears highly concentrated with a bright central bulge that dominates its overall appearance. The galaxy exhibits a smooth luminosity profile, with light intensity decreasing gradually from the center outwards. No distinct spiral arms or prominent dust lanes are discernible. There may be a very faint hint of a diffuse halo surrounding the central region, but it lacks any clearly defined structures. The galaxy displays a slightly reddish-orange hue, indicative of an older stellar population and potentially lower levels of current star formation. There is no evidence of ongoing major merging activity or significant tidal disturbances in the immediate vicinity. The object appears essentially undisturbed and isolated within its environment.
