The galaxy exhibits a clear spiral structure. The spiral arms appear tightly wound and are the dominant feature of this galaxy. It displays a small bulge relative to the disk, and the presence of a bar structure is indicated, although not strongly defined. There is no evidence of significant ongoing merger activity or major disturbances.

The overall color of the galaxy suggests a mix of stellar populations, with a concentration of older, redder stars in the central bulge and younger, bluer stars populating the spiral arms. The disk component is seen nearly edge-on.