The breakup of the mean scatter of visual classification metrics for galaxies at 0.5 <z< 2.5 binned by their final mean metric value. The mean scatter for a galaxy is defined as the average absolute value of the difference of the metric between pairs of classifiers for that galaxy. Galaxies with larger scatter have a larger level of disagreement between the individual visual classifications. The relative number of galaxies in four ranges of scatter are shown, represented by lighter to darker grayscale towards increasing scatter. Galaxies are binned by the final interaction metric (IM, left panel) and the final clumpiness metric (CM, right panel).