The galaxy presents as an elongated, edge-on disk galaxy. A prominent central bulge dominates the galaxy's core, exhibiting a yellowish-orange hue, indicative of an older stellar population. Surrounding the central bulge is a flattened disk, displaying a bluer tint. This suggests a younger stellar population within the disk, where star formation is likely more active. The disk appears relatively smooth with no obvious spiral arm structures. There is no visible sign of major mergers or significant disturbances in the galaxy's morphology. The outer regions of the disk appear slightly fainter and less defined. There is a suggestion of dust lanes obscuring the bulge slightly.
