The observed galaxy presents an edge-on disc morphology. A prominent dust lane bisects the galaxy, obscuring the central bulge and a significant portion of the galactic disc. The disk is relatively thin with a noticeable warp. Color gradients are visible; the outer regions of the disk appear bluer, possibly indicating younger stellar populations. The central region appears redder, suggesting older stars or increased dust concentration. There is little evidence of spiral arm structure. The galaxy exhibits no obvious signs of a recent major merger.
