The galaxy exhibits a prominent disk structure with observable spiral arm features. These spiral arms appear tightly wound. The central bulge of the galaxy seems relatively moderate in size compared to the overall disk. There is no readily apparent strong bar structure, nor is there evidence of any ongoing major merger activity. Some minor disturbances are possibly suggested within the galactic structure. A substantial amount of star formation appears to be happening within the galaxy. The galaxy is likely viewed at a relatively low inclination angle.
