The galaxy presents as a spiral type, observed at a redshift indicating a considerable distance. The morphology indicates a prominent, but not dominant, central bulge from which spiral arms emanate. These arms appear to be well-defined and tracing around the bulge in a generally consistent fashion. There is evidence of flocculent spiral structure distributed throughout the disk. The arms appear to be wound moderately tightly, but not exclusively so. The color gradient suggests star formation within the spiral arms, as evidenced by the blueish and white hues present, while the bulge exhibits a yellow-red shift indicating an older stellar population. No significant tidal features or signs of major mergers are apparent, though some minor disturbances may exist. Based on the arm characteristics, it is likely that the spiral galaxy has two primary arms. The presence of a faint bar structure cannot be ruled out based on visual inspection. The galaxy's overall form appears relatively undisturbed, suggesting a stable, though active, evolutionary stage.
