This galaxy presents as a relatively compact and spheroidal structure. The light distribution suggests a smooth, elliptical morphology, with little evidence of spiral arms or a prominent disk. Color gradients are present. The core exhibits a concentration of light that appears slightly more yellow. The outer regions display a bluer hue, hinting at the potential presence of some younger stellar populations residing in the outskirts, though this appears to be a minor component. There is no evidence of any major disturbances or ongoing merging activity.
