The galaxy presents as an edge-on spiral, exhibiting a flattened disk structure. The disk appears relatively smooth, with a subtle central bulge that seems elongated along the disk's major axis. Light from the galaxy suggests a population of young, hot stars, indicative of ongoing star formation, primarily concentrated within the galactic disk. The galaxy shows a slight warp or tilt at one end of the disk. There is no sign of a prominent dust lane, nor any major mergers. This is most likely a smaller galaxy undergoing star formation at a moderate rate.
