The galaxy presents as a somewhat elongated, disk-like structure. There appears to be a central bulge, brighter than the surrounding regions. Faint spiral arm features might be present within the disk, although resolution limitations make this uncertain. The disk itself is observed at an oblique angle. The overall color of the galaxy seems to be slightly blue, suggesting some ongoing star formation. The galaxy does not seem to be undergoing a major merger, though there could be some minor gravitational disturbances, perhaps due to a small companion. The galaxy is relatively small in apparent size and is observed at a distance, given the measured redshift.
