Nonparametric morphological indicators for each of the galaxies in our sample as a function of wavelength, and for the stellar mass, dust mass, and SFR maps. The different panels correspond to the half-light radius R_half normalized by the optical R₂₅ diameter (top left), the concentration index (top right), the asymmetry index (middle left), the smoothness index (middle right), the Gini coefficient (bottom left), and the M₂₀ indicator (bottom right).