The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a noticeable central bulge, with the overall shape appearing somewhat elongated or cigar-shaped rather than perfectly spherical. The color profile suggests a concentration of older stellar populations, indicated by the yellowish to reddish hue of the central region. There is minimal evidence of spiral arms or significant dust lanes. The galaxy displays no obvious signs of major mergers or significant tidal disturbances.
