The galaxy presents as a flattened, disk-shaped system, oriented nearly edge-on relative to the observer. The central bulge is prominent, appearing bright and concentrated with a yellowish-white hue, suggestive of an older stellar population. Moving outward from the bulge, the disk exhibits a bluer color, implying more active star formation. The disk appears thin and elongated, with some subtle dust lane structures visible along the plane of the disk. The galaxy shows no obvious signs of major mergers or strong tidal interactions, maintaining a relatively undisturbed morphology.
