The galaxy presents as a highly inclined, likely late-type spiral system. It displays a prominent central bulge that dominates its overall luminosity. The galaxy's disk is visible as a flattened structure extending from the bulge. Although indistinct, the disk appears to contain some degree of substructure, suggesting the presence of spiral arms, although they are difficult to resolve given the viewing angle.

The dust lane, characteristic of edge-on spiral galaxies, may be present but not clearly identifiable. The galaxy exhibits a color gradient, with the bulge appearing yellower than the disk, indicative of an older stellar population. The morphology suggests that the galaxy has likely experienced internal processes that led to the formation of a significant bulge component.
