This galaxy presents as a near edge-on spiral. A prominent dust lane bisects the galaxy, obscuring the central bulge. This obscuration suggests a significant amount of interstellar dust within the galactic disk. The central bulge appears relatively small and has a boxy morphology. The disk is elongated, extending significantly from the central bulge. Some patchiness and irregularities are apparent within the disk, hinting at ongoing star formation regions and possibly minor gravitational interactions within the galaxy itself.
