The galaxy presents a moderately inclined disk morphology. Spiral arm structures are discernible, appearing somewhat tightly wound around the galactic center. The central bulge appears small to moderate in size relative to the overall disk. There is no obvious bar structure evident. The galaxy does not exhibit any major signs of disturbance or ongoing merging activity, though minor distortions cannot be ruled out based on this image alone. Star formation appears to be present. The galaxy has an estimated size of 6.2 kpc.
