The galaxy presents as a generally smooth, elliptical form with a slightly elongated shape. A central bulge exhibits a bright, concentrated luminosity, transitioning to a more diffuse halo. The dominant color appears to be yellowish-orange, suggesting an older stellar population. The lack of distinct spiral arms or dust lanes indicates a relatively quiescent system, potentially with a low star formation rate. There are no obvious signs of tidal disturbances or major mergers, though subtle asymmetries hint at a possible minor interaction in the past.
