The galaxy presents as a disk galaxy, observed at an oblique angle close to edge-on, but where the full structure of the disk is visible. The disk itself exhibits a mottled texture, likely indicating regions of varying stellar density and ongoing star formation. There is some blue tint to the galaxy. A bar-like structure is visible across the major axis of the galaxy, adding to the disk's complexity. A central bulge is present, though appears to be only a relatively small contribution to the overall luminosity of the galaxy. Faint spiral arm structures appear to emanate from the bar and extend outwards into the disk, though these arms are not particularly well-defined. The outer regions of the disk fade into the background, suggesting a gradual decrease in stellar density with increasing radius. 
