The galaxy presents as a spiral, viewed at an oblique angle. It exhibits a moderately sized central bulge that appears elongated. Two prominent spiral arms emanate from the core region, appearing somewhat tightly wound closer to the center and gradually becoming looser as they extend outward. The arms are distinctly delineated and show evidence of active star formation, indicated by the presence of blue-tinged regions. The overall color of the disk suggests a relatively young stellar population. There is also a faint stellar halo visible. There is a suggestion of a bar-like structure across the central bulge, although it is not highly pronounced. There are no obvious signs of any major mergers occurring with another galaxy, but the asymmetry in the outer disc could indicate some sort of minor tidal interaction.
