The galaxy presents a clear spiral structure, with prominent arms extending from a central bulge. The spiral arms are somewhat fragmented. Evidence suggests moderate ongoing star formation within the disk, as indicated by the blueish hue along the spiral arms.

The central bulge appears relatively moderate in size and presents a yellowish color. It is not possible to tell how strong the galaxy's bar is with this image, but it appears elongated. No signs of active galactic nuclei activity are evident from visual inspection.
