The galaxy presents as a relatively smooth, elliptical-like structure. The light distribution appears centrally concentrated, with a gradual decrease in surface brightness towards the outer regions. Color gradients within the galaxy appear subtle, with a slightly redder core transitioning to somewhat bluer outskirts, although this is not pronounced. The overall morphology suggests a galaxy undergoing or having completed a process of quiescence, potentially exhibiting lower rates of ongoing star formation. There is no discernible disk component, spiral arms, or distinct dust lanes, indicating a more evolved or spheroidal system. No signs of major mergers or tidal disturbances are readily visible. 
