Evolution of the fractions of different morphological types in rest-frame ∼0.8 − 1 μm as a function of stellar mass and redshift. Filters F200W, F356W, and F444W are used to infer galaxy morphology in the redshift bins 0 < z < 1, 1 < z < 3 and 3 < z < 6, respectively. Each panel shows a stellar mass bin as labeled. Top row: fractions in four morphological classes: spheroids (red), disks (blue), bulge+disk (orange), and peculiar or irregular (green). Middle row: fractions in two broad classes: disk dominated (blue) and bulge dominated (red). Bottom row: fractions in two broad classes: regular (blue) and disturbed (green).