The galaxy presents as a lenticular-like structure. It exhibits a smooth, centrally concentrated bulge that appears relatively bright and featureless, indicative of an older stellar population. Surrounding the bulge is a fainter disk component. The disk does not show defined spiral arms or distinct dust lanes, which contributes to the smooth overall appearance. The disk appears slightly more elongated. Faint blueish color is slightly visible in areas surrounding the central bulge, potentially suggesting some on-going but subdued star formation. There are no obvious signs of interactions or major disturbances, however some of the overall shape of the galaxy is not perfectly spherical and may be experiencing minor interaction. Overall the galaxy seems to be relatively massive. 
