The galaxy presents as a largely featureless, elliptical-like object with a smooth light distribution. The central region exhibits a higher luminosity, with a color gradient transitioning outwards to a redder, more diffuse halo. No distinct spiral arms or bar structures are discernible. The overall shape appears moderately rounded but leans slightly towards being in between round and cigar shaped. There is no visually apparent evidence of ongoing major mergers or significant tidal disturbances, although minor disturbances cannot be ruled out. The color indices suggest a relatively evolved stellar population and low star formation rate.
