The object appears to be a spiral galaxy, observed at a redshift that places it at a considerable distance. It presents a disk-like structure, viewed at an angle that allows us to see some internal structure. There appears to be distinct spiral arm structure, though they are not exceptionally well-defined, and may be considered somewhat flocculent. A central bulge is present and appears to be of moderate size relative to the overall disk. The disk exhibits a general blue hue while the bulge has a more reddish-yellow color, suggestive of older stellar populations or significant dust obscuration. The galaxy is approximately 10 kpc in radius. There is no obvious indication of a major ongoing merger, though there is a possibility of some minor disturbance in the disk. The object is actively forming stars. Bar structure exists but is ill-defined.