The galaxy presents as an elongated, edge-on spiral type. It is characterized by a distinct, central bulge exhibiting a yellowish-white hue, suggesting an older stellar population. This bulge transitions into a flattened disk structure. The disk component is primarily bluish, indicative of ongoing star formation and a younger, hotter stellar population. A thin, dark dust lane is not easily visible. Irregular structures and extensions are present in the lower portion, perhaps resulting from gravitational interactions or minor disturbances. The galaxy is relatively faint and of moderate apparent size. No prominent signs of a major ongoing merger are observed.
