The galaxy presents as a relatively small, faint, edge-on spiral. A prominent dust lane bisects the galaxy, causing significant obscuration of the central bulge. The bulge appears relatively large and rounded, with the dust lane running horizontally across its mid-section. The disk is thin and elongated, with a noticeable color gradient extending from the bulge towards the outer edges. The overall color is reddish. There is no obvious sign of recent or ongoing merger activity or significant tidal disturbances. The central bulge exhibits a smooth luminosity profile, suggesting a relatively old stellar population. The observed morphology indicates a quiescent system with low star formation rates.
