The galaxy presents as a moderately bright, elliptical-shaped object. It exhibits a smooth, concentrated central bulge that appears almost spherical. The outer regions of the galaxy fade gradually into the background sky. Color gradients are subtle, with a slight bluing towards the outer edges. There are no discernable spiral arm structures or dust lanes visible. The galaxy appears relatively undisturbed, showing no strong evidence of recent mergers or tidal interactions. The overall light distribution suggests a mature stellar population, with possible ongoing, though limited, star formation activity in the outer regions.
