The galaxy presents as a relatively smooth, elliptical or lenticular system. It exhibits a concentrated central bulge with a diffuse halo extending outwards. The color profile suggests an older stellar population, dominated by yellow and red hues. No spiral arm structure or significant dust lanes are visible. The overall morphology is largely undisturbed, showing no signs of ongoing major mergers or tidal distortions, though there may be minor disturbances. It appears relatively round, without a highly elongated or cigar-shaped structure.
