The galaxy presents as a centrally concentrated, elliptical structure with a smooth, diffuse light distribution. The core exhibits a bright, yellowish hue, indicating an older stellar population. The outer regions display a gradual decrease in surface brightness. While appearing mostly rounded, there is a subtle elongation along one axis. No distinct spiral arms or significant dust lanes are apparent within the observable structure. The galaxy shows no obvious signs of major mergers or significant tidal disturbances based on visual inspection. The overall morphology suggests a relatively evolved system, potentially a lenticular or early-type spiral galaxy.
