The galaxy presents as a spiral type, exhibiting a distinct disk structure. Prominent spiral arms are observed, though difficult to define their number, the winding appears relatively tight around the galactic center. A bulge is visible, representing a moderate portion of the overall galactic luminosity. The galaxy's overall structure doesn't show any obvious signs of significant tidal disruption, suggesting a relatively quiescent merger history. Some star forming regions are observed in the spiral arms. The inclination is rather large and this galaxy is close to edge-on. There is no central bar that is easily visible, and no indication of interaction with a nearby galaxy.