The galaxy presents an elliptical morphology, exhibiting a smooth and centralized light distribution. The core region is significantly brighter and appears yellowish in color, possibly indicating an older stellar population. Proceeding outwards, the galaxy fades into the surrounding background, displaying a decreasing surface brightness. There appears to be little to no visible spiral arm structure or prominent dust lanes, suggesting a lack of significant ongoing star formation. A slight degree of asymmetry is present in the outer regions, but not enough to suggest major disturbances, such as an ongoing merger.
