The galaxy presents as an elongated, edge-on spiral. A prominent dust lane bisects the galaxy along its major axis, obscuring a significant portion of the central bulge. The bulge itself appears relatively small and featureless. The disk of the galaxy is thin and appears undisturbed, showing no signs of recent major mergers or tidal interactions. There is a faint, diffuse halo extending beyond the visible disk. The galaxy exhibits a color gradient, with the central regions appearing slightly redder compared to the bluer outer disk, suggestive of older stellar populations near the bulge and ongoing star formation in the disk. The galaxy's disk appears relatively smooth overall, indicative of a generally stable morphology.