The galaxy appears as a flattened, disk-shaped structure, viewed nearly edge-on. A prominent central bulge dominates the galaxy's core, exhibiting a yellowish hue, likely indicating an older stellar population. Fainter, bluer light extends along the plane of the disk, suggestive of ongoing star formation. The disk appears relatively smooth, with minimal visible spiral arm structure. There is a slight asymmetry to the disk, with one side appearing more extended or disturbed than the other. No clear signs of a major merger or significant tidal disruption are apparent, though minor disturbances cannot be ruled out. Overall, the galaxy presents as a relatively quiescent, late-type disk galaxy.
