The galaxy presents as a largely smooth, elliptical-like structure, exhibiting a concentration of light towards its center. The color profile indicates an older stellar population, leaning toward redder wavelengths across the galaxy. There is minimal to no indication of spiral arms or significant dust lanes. The galaxy appears relatively undisturbed, without any visible signs of ongoing major mergers or tidal distortions. A slight deviation from perfect roundness is observed, though the overall shape remains predominantly spheroidal. The outer regions gradually fade into the background, suggesting a diffuse halo.
