The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that fades gradually into the outer regions, with no discernible spiral arm structures or distinct dust lanes. The overall color appears bluish, possibly indicating the presence of relatively young, hot stars, although the intensity of star formation seems subdued. The galaxy appears to be fairly symmetrical, with no obvious signs of major recent mergers or significant tidal disturbances, though minor disturbances cannot be ruled out. It is a relatively compact galaxy.
