The galaxy appears to be a spiral galaxy, observed at a redshift that suggests an intermediate distance. It exhibits clear signs of disturbance, likely due to an ongoing or recent merger event.

The morphology shows a prominent disk with spiral arms. These arms appear somewhat disrupted and asymmetrical. The color distribution indicates a relatively high level of star formation, with some areas showing a bluer hue, indicative of younger stellar populations.

A significant portion of the galaxy's light is concentrated in what seems to be an ongoing interaction/merger. There are distinct features indicating a complex gravitational interaction, such as tidal tails or bridges of material extending away from the main galactic body. The overall structure is not clearly defined, indicating an advanced stage of the merger.

The galactic bulge is not very prominent, suggesting a disk-dominated morphology. There is no strong presence of a central bar feature. The galaxy exhibits high star formation rates, which could be a result of tidal interactions or the merger.
