Non-parametric rest-frame optical and near-infrared morphology of the NIRCam-SMGs. We show the Gini and M₂₀ plane (left). The dashed black lines indicate the division between Mergers, Elliptical and Disc galaxies as defined by Lotz et al. (2008). In the middle panel we show the correlation between clumpiness (S) and concentration (C₂₈), with the parameter space of local galaxies from Conselice et al. (2003) overlaid. Finally, in the right panel we show the asymmetry (A) concentration (C₂₈) plane with dashed lines showing the distinction between Mergers, Disc, Intermediate and Ellipticals from Bershady et al. (2000) and Conselice et al. (2003). In all three panels, the optical and near-infrared samples occupy the region with disc-like morphology.