This galaxy exhibits a disk morphology, though the viewing angle makes it difficult to ascertain if the galaxy is truly edge-on. There is evidence of spiral arm structure. Although the resolution is limited, the presence of two arms can be inferred. The winding of the spiral arms appears relatively open. The galaxy possesses a central bulge. The bulge appears to be of moderate size. There may be a weak bar structure. The galaxy appears to be relatively undisturbed, with no significant signs of major mergers or tidal interactions. There are no obvious signs of star formation activity visible. 
