The galaxy presents as a fairly smooth, elliptical-like structure with a concentrated central bulge that is bright and yellow. The overall shape appears largely regular and rounded. There is little to no evidence of spiral arms or a distinct disk component; instead, it exhibits a gradual decrease in luminosity from the core outwards. The halo is relatively smooth and extends evenly in all directions, with a faint red hue, suggesting an older stellar population. There are no clear signs of recent or ongoing major mergers or significant tidal disturbances in this image. Overall the galaxy appears as a fairly undisturbed, isolated system.
