The object appears to be a spiral galaxy, observed at a redshift of approximately 0.25. Its apparent size indicates a substantial physical diameter in kiloparsecs. The galaxy exhibits prominent spiral arms. They seem to be relatively tightly wound toward the galactic center, however, they also exhibit some extended and more loosely wound sections. There is evidence of a central bulge region and it appears to be moderate in size.

There is no evidence of any ongoing merging activity, and the disk does not appear to be edge-on from our perspective. The spiral structure appears to consist primarily of two distinct arms, though it's hard to tell given the relatively compact nature of the spiral pattern. The color distribution suggests active star formation within the spiral arms. The overall shape appears to be relatively undisturbed.
