The galaxy presents as an edge-on spiral, with a prominent dust lane bisecting its major axis. The central bulge appears elongated and relatively smooth. The disk component displays a diffuse, somewhat irregular morphology, exhibiting a higher degree of concentration towards the central bulge. Faint blue light is visible within some regions of the disk, but the overall color indices suggest a predominantly older stellar population, especially towards the bulge. There appear to be some minor tidal disturbances present in the disk, as well as some degree of irregular morphology.
