The galaxy presents as a highly inclined, edge-on spiral galaxy. It exhibits a prominent, centrally located bulge, appearing smooth and rounded. The disk is clearly visible as a flattened structure extending from the bulge. There is some indication of obscuring dust lanes. There are signs of possible disturbances in the disk, however the galaxy is not currently undergoing any major merging events. Star formation appears to be relatively low. The estimated size of the galaxy is approximately 9.2 kpc. 
