The galaxy presents as a relatively smooth, elliptical structure. Its core exhibits a concentrated, bright yellowish-white glow, suggesting an older stellar population. Moving outward from the core, the light diffuses into a broader, less intense halo with a subtle reddish hue. The overall shape leans towards being somewhat rounded, but there is a moderate deviation from perfect circularity. There are no apparent signs of a prominent disk or spiral arms. While the galaxy appears largely undisturbed, there are hints of minor irregularities in the outer regions, possibly indicating past interactions or minor disturbances. The smooth light distribution implies a galaxy that has largely completed the merging process or has not experienced a major merger event in its recent history.
