The galaxy presents an elongated, disk-like structure viewed at a high inclination. The central bulge exhibits a yellowish-orange hue, suggesting an older stellar population. Moving outward from the center, the disk displays a bluer tint, potentially indicative of ongoing or recent star formation. There are subtle hints of spiral arm structures within the disk, though they are not sharply defined. The overall morphology appears relatively undisturbed, lacking prominent signs of tidal interactions or major mergers. The galaxy appears to be relatively smooth and only displays minor disturbances.
