The galaxy presents a predominantly smooth morphology, suggesting an elliptical classification is plausible. It exhibits a moderately elliptical shape, appearing somewhat flattened but not strongly elongated. The central region displays a bright, concentrated core, indicating a high stellar density. Moving outwards from the core, there is a gradual decrease in brightness, forming a diffuse halo. The overall color profile indicates a significant presence of older stellar populations. While predominantly yellow-orange, a subtle green tint can be observed which may reflect ongoing low-level star formation or a presence of ionized gas. There is no apparent spiral arm structure, and the galaxy appears relatively undisturbed, with no signs of major mergers or tidal interactions. Faint disturbances are potentially observable in the outer regions, but they remain unconfirmed due to their subtlety. The galaxy appears isolated within its immediate environment.
