The galaxy exhibits a clear spiral structure, with at least two discernible arms. The arms appear somewhat flocculent and are moderately wound. There is a central bulge that appears relatively small compared to the overall disk size. A faint bar-like structure seems to exist within the central region. There is evidence of ongoing star formation within the spiral arms, indicated by bluer colors. The galaxy disk is oriented close to face-on. There is some visual irregularity in the disk that may be a sign of a minor disturbance.
