This galaxy appears to be a spiral galaxy, observed at a redshift that places it at a considerable distance. The galaxy presents a disk-like structure, oriented face-on relative to our line of sight. Spiral arms are visible, showing moderate winding. Two main arms are distinguishable extending from a central region with moderate bulge.

The overall color of the galaxy suggests a mix of stellar populations, with bluer hues apparent within the spiral arms, potentially indicating ongoing star formation. The central bulge appears more yellow, suggestive of older, redder stellar populations. There is some asymmetry to the arms. No obvious major mergers or disturbances can be identified.
