The object appears to be a spiral galaxy, observed at a redshift that places it at a considerable distance. The galaxy exhibits a disk-like structure with prominent spiral arms. Two main spiral arms are discernible, displaying a medium winding. There is evidence of flocculent structure within the arms, indicating active star formation. 

A central bulge is present, with a moderate size relative to the disk. A bar structure is present in this galaxy.

There are no signs of any major tidal disturbance or merger events.