The galaxy presents as a largely featureless, elliptical-like object with a smooth light distribution. It exhibits a concentrated central bulge with a noticeable radial gradient, transitioning from a bright, yellowish core to a more diffuse, reddish outer halo. The overall shape is generally round. There is no evidence of spiral arms, dust lanes, or other distinct morphological features typically associated with late-type galaxies. The galaxy appears relatively isolated, with no signs of major tidal distortions or ongoing mergers. There are hints of minor disturbances; however, the galaxy seems to be stable. It has very little star formation.