The galaxy presents as a spiral type, observed at a moderate redshift. Disk morphology is readily apparent, oriented roughly face-on. Distinct spiral arms are visible; most appear tightly wound, defining a grand design structure. The arm count is likely two, although the number is somewhat uncertain due to the tightness of the spiral arms. A central bulge is present, appearing moderate in size, with a relatively small, bright core. A weak bar feature is also a possibility. The color gradient suggests ongoing star formation within the spiral arms. There are no obvious signs of major merging activity or significant tidal disturbances, however, there appears to be a minor companion nearby, and some indications of minor disturbances.
