The galaxy presents as a relatively compact structure. Its overall shape is elliptical, appearing somewhat elongated rather than perfectly spherical. A smooth light distribution characterizes its morphology, with a bright central bulge. The concentration of light towards the center is evident, with intensity gradually decreasing outward into the fainter edges. There is a faint disk structure as it is not perfectly elliptical. There is no sign of major disturbances such as tidal tails or obvious signs of recent mergers. No distinct spiral arms or prominent dust lanes are observed. The colour profile indicates older stellar populations are more prominent, with redder colours becoming more apparent with distance from the center of the galaxy. The morphology of the galaxy indicates a moderate mass system, with a low rate of star formation. 
