The galaxy presents as a relatively small, edge-on spiral system. A distinct, although somewhat faint, dust lane is visible, bisecting the galaxy along its major axis, indicating the presence of a galactic disk. The overall color appears bluish, potentially suggesting ongoing star formation, although the image resolution limits precise determination of distinct star-forming regions. The bulge appears small and ill-defined. There does not appear to be any evidence of major mergers or significant tidal disturbances. The galaxy has a notably extended HI profile.
