The galaxy presents as an elongated, edge-on spiral with a prominent central bulge. The bulge exhibits a color gradient, appearing more yellow-orange towards the center, potentially indicating an older stellar population. Fainter, bluer hues extend from the bulge into the disk, suggesting areas of more recent star formation. The disk shows indications of dust lanes or patchy structures, adding to the overall complexity of the galaxy's morphology. No obvious signs of major mergers or strong tidal disturbances are visible.
