The galaxy appears to be a spiral galaxy, observed at a moderate redshift. The galaxy exhibits a distinct disk structure with prominent spiral arms. These arms seem to have a fairly defined winding pattern, neither extremely tight nor overly loose. The arms appear to contain areas of active star formation regions, indicated by the presence of a blueish hue in the spiral arms. The central bulge of the galaxy seems significant in size, but not exceedingly dominant. There are no obvious signs of major ongoing mergers, but there could be evidence of minor disturbances in the galaxy's morphology, potentially indicating past interactions. The orientation is such that the galaxy is viewed at close to face-on. Dust lanes may be present within the spiral arms, but the resolution limits further analysis of dust distribution.
