The galaxy appears to be a spiral galaxy, observed at a redshift that places it at a considerable distance. Its disk is oriented at an oblique angle to our line of sight. The spiral arms are well-defined and loosely wound, tracing a grand design pattern. Two main arms are distinctly visible, although there is a degree of patchiness. The central bulge shows a moderate size relative to the overall galactic disk. A bar structure is possibly present, spanning a fraction of the bulge’s diameter. Star formation activity seems to be prevalent within the spiral arms as evidenced by the clumpy regions. There is no clear evidence of a major ongoing merger, but some minor morphological disturbance or irregularity might be present in the disk.
