This galaxy presents as a relatively bright, edge-on disk galaxy. It exhibits a clear, centrally concentrated bulge. Dust lanes are visible, obscuring a portion of the bulge and inner disk, adding to the redness of the galaxy. The disk component appears prominent and is relatively thin, though a slight warping is possible. Based on the dust lane structure, the galaxy is likely a spiral, though the arms cannot be resolved from this viewing angle. The bulge appears somewhat elongated or boxy, but may also be rounded. Overall, the galaxy exhibits features consistent with ongoing star formation, with the reddish color possibly indicating both dust and older stellar populations. There are no obvious signs of significant interactions or major mergers.