This galaxy appears to be a spiral galaxy, observed at a redshift indicating a substantial distance. The spiral arms are loosely wound and defined, displaying a prominent blue hue, which suggests ongoing star formation within these regions. The galaxy exhibits a weak bar structure running through its central region, potentially influencing the morphology of the spiral arms. The central bulge is relatively small and does not dominate the galaxy's overall structure. There may be a minor interaction or disturbance visible, but the galaxy does not present the appearance of a major ongoing merger, despite some noticeable asymmetry. The disk is not viewed edge-on, presenting a face-on or near face-on orientation. The galaxy presents a smooth disk with some defined, loose spiral structures.
