The galaxy presents as a spiral with a noticeable, yet not overwhelmingly dominant, central bulge. The spiral arms are prominent and well-defined, extending outwards from the core region. There appears to be ongoing star formation occurring within these arms, as indicated by the blueish-white colors and clumpy structures. There is some indication of a weak bar structure. There is no apparent signs of major interactions with another galaxy. The spiral arms do not appear symmetric, and some appear less tightly wound than others.
