The galaxy presents as an elongated, edge-on or highly inclined spiral or lenticular galaxy. The dust lane is subtle, running along the major axis and obscuring light from the central bulge. Star formation appears to be occurring throughout the disc, traced by regions of bluer light. The bulge appears relatively small compared to the disk. The galaxy has a flattened, disk-like morphology. There appears to be no obvious signs of a strong bar or spiral arms.
