The galaxy presents as a spiral, with a relatively small bulge component compared to the overall disk. Spiral arms are prominent, exhibiting a tightly wound morphology. There appears to be ongoing star formation, given the bluer hues observed in the spiral arms, possibly indicative of younger stellar populations. The overall structure seems relatively undisturbed, with no significant signs of major mergers or tidal disruptions, although some minor asymmetries are present. The disk is not perfectly edge-on. A bar structure is possibly present, but subtle.
