The object presents as a spiral galaxy, viewed at a moderate angle relative to its disk. It exhibits prominent, loosely wound spiral arms that dominate the galactic structure. These arms appear somewhat flocculent, with a patchy distribution of star formation regions. The central bulge is relatively small compared to the overall disk size.  There is some indication of a bar-like structure extending through the central region, though it is not strongly defined. The galaxy lacks any obvious signs of a major ongoing merger, although subtle morphological disturbances suggest possible minor gravitational interactions. Overall, the galaxy appears to be a relatively undisturbed spiral with ongoing star formation, likely indicative of a late-type spiral classification. The observed redshift places this galaxy at a considerable distance.
