The galaxy presents a generally smooth morphology, with no immediately apparent spiral arm structure or bar. It appears elliptical in shape but is close to round. There is a distinct color gradient; the core region exhibits a reddish-orange hue which gradually transitions to a greenish-yellow at the outer edges. The color likely indicates variations in stellar populations and dust content. The galaxy appears relatively undisturbed, with no obvious signs of ongoing or recent major mergers or tidal interactions. There are no other signs of disturbances in the disk.
