The galaxy presents a largely smooth morphology, appearing as a singular, concentrated structure. Its overall shape is generally round. The core region exhibits a distinct yellowish hue, suggesting an older stellar population. The outer regions of the galaxy display a subtle greenish tint, possibly indicative of some ongoing, albeit limited, star formation. There are no readily apparent tidal features or significant distortions to suggest recent major merger activity. The overall structure points towards an elliptical or S0 galaxy classification.
