The galaxy presents as a relatively small, edge-on spiral, displaying a prominent disk. A distinct bulge is visible at the galactic center, appearing somewhat rounded. The disk exhibits a subtle but perceptible warp. There is an indication of asymmetry, with one side of the disk displaying a slight extension or disruption. Evidence suggests minimal ongoing star formation. Possible minor interactions with other galaxies or tidal effects may be the cause for the asymmetry.
