The galaxy presents as an edge-on disk galaxy, with a notable central bulge. The bulge appears to be predominantly rounded in shape. A faint disk is observable, extending outwards from the central bulge. There does not seem to be any indication of spiral arms that are typically found in galaxies. The overall color index suggests a relatively high concentration of older stars. There is no major evidence of current, ongoing star formation in the area surrounding this galaxy, nor does the galaxy show sign of recent merger activity, although minor disturbance cannot be ruled out. The galaxy appears to be isolated.
