The observed galaxy appears to be a spiral galaxy, observed at a redshift indicative of relatively low cosmological distance. The structure is dominated by a flattened disk, oriented at a significant inclination relative to the line of sight. Two distinct spiral arms are apparent, exhibiting a somewhat loose winding. The central bulge is relatively small and not dominant. There appears to be a bar structure present. The overall color suggests ongoing star formation, with the spiral arms appearing bluer. No significant signs of major mergers or tidal disturbances are evident, though there are subtle signs of minor disturbances.
