The galaxy presents as an edge-on spiral or lenticular galaxy with a prominent bulge. The central bulge exhibits a smooth, spheroidal morphology with a concentrated luminosity. The disk is thin and elongated, showing evidence of dust lane obscuration across the major axis. There is little evidence of current star formation visible in the disk. The overall colour index suggests a stellar population dominated by older stars, consistent with a low specific star formation rate. The galaxy does not exhibit any obvious signs of ongoing mergers or major tidal disturbances. The bulge appears to be rounded rather than boxy in nature.
