Observed is a spiral galaxy at a redshift of approximately 0.23, indicating an appreciable distance. The galaxy exhibits a prominent disk structure with tightly wound spiral arms. These arms display a loose morphology and trace the outline of the disk, suggesting ongoing star formation activity. The galaxy possesses a notable central bulge, although it is not overwhelmingly dominant. Indications of a bar structure are present, but appear to be relatively weak. There is no obvious signs of tidal disturbances or ongoing major merging events, and only a slight indication of minor disturbances.
