The galaxy presents as a barred spiral with a central bulge. The bar structure appears prominent, spanning a significant portion of the galactic disc. The spiral arms are tightly wound and are rather symmetric on either side of the bar. There are two dominant arms, one on each side. The disk component shows a significant degree of internal structure, with some bluer regions indicating areas of potential star formation. The bulge itself appears relatively small, in comparison to the disk. There is no obvious signs of major mergers occurring, but some minor disturbances or tidal features are present. The overall color suggests a system undergoing active star formation. The galaxy is not viewed edge-on, but at a shallow angle.
