The galaxy presents as an edge-on spiral system. A dust lane bisects the disk, obscuring the central bulge region. The bulge appears relatively small and elongated, but the inner regions have some yellow emission, perhaps from a population of older stars. The galaxy disk itself exhibits some mottled texture, with some bluer patches indicating the presence of star-forming regions, although they are largely redder in color suggesting on average a low star formation rate. The galaxy shows an asymmetry, with one side appearing more extended, possibly due to tidal interactions or a lopsided disk structure. There is no distinct nuclear point source visible, and the morphology is indicative of a relatively undisturbed system.
