The galaxy presents as a fairly smooth, elliptical-like object with a concentrated central bulge and a diffuse halo. It is largely featureless. The color distribution indicates a redder core, possibly indicating an older stellar population or significant dust obscuration. The outer regions appear somewhat bluer, potentially suggestive of more recent star formation in the outskirts, although the overall color is suggestive of a red sequence galaxy. There is no apparent disk structure or spiral arms visible. The galaxy exhibits a high degree of symmetry, and there are no signs of major disturbances or ongoing mergers. The morphology suggests a relaxed system.
