The galaxy appears as a disk-shaped system viewed nearly edge-on. A central bulge component is present, exhibiting a yellowish-white hue, suggestive of an older stellar population. The disk itself displays a bluer tint in the outer regions, potentially indicative of ongoing star formation. Some irregularities along the disk's edge are visible, though there is no immediately obvious sign of a major ongoing merger. Some signs of a minor disturbance are present. The galaxy's disk appears relatively smooth in appearance, lacking prominent spiral arm structures. Overall, the galaxy presents characteristics consistent with a star-forming spiral galaxy observed at a considerable distance.
