This galaxy exhibits a flattened, elongated morphology, suggesting it is likely a spiral galaxy viewed at a high inclination or an elliptical galaxy. The light distribution is smooth and centrally concentrated, with a subtle color gradient, appearing more yellow/orange towards the core and transitioning to a bluish hue in the outer regions. The structure suggests a relatively old stellar population in the central bulge, indicated by the yellower color, with possible ongoing star formation in the disk, as suggested by the bluer outer regions. There's no clear evidence of strong spiral arm structure, but this may be due to the viewing angle or the limitations of the image resolution. The galaxy appears relatively undisturbed, without obvious signs of a recent major merger or tidal interactions.
