The galaxy appears to be a spiral galaxy, viewed at a slight angle from face-on. Its shape is elongated, showing a disk-like structure with a central bulge. The spiral arms are well-defined, displaying a loosely wound pattern. We can clearly see that the disk component dominates over the bulge component. There are indications of ongoing star formation within the spiral arms, with a mottled appearance and some regions of bluer light, suggesting the presence of young, hot stars. There is some evidence of a bar structure. The color of the galaxy is generally bluish, with hints of redder light concentrated towards the center, which is to be expected with a spiral galaxy at this redshift. There are some signs of a possible interaction or minor disturbance.
