The galaxy presents as an edge-on spiral or lenticular galaxy. A prominent central bulge is observed, with a color gradient suggestive of an older stellar population. A thin, faint disk extends outwards on either side of the bulge. Evidence of dust lanes is present, subtly obscuring parts of the galactic disk. The overall structure appears relatively undisturbed with no significant signs of tidal interactions or major mergers. The bulge appears to be more rounded in shape. Subtle asymmetric features may be present within the disk. 
