Illustration of the deconvolved surface brightness profiles. The left two panels illustrate the intrinsic profiles obtained from high-resolution images of nearby galaxies, featuring ESO 112-005 at the top and NGC 12 at the bottom, respectively. The panels in the subsequent columns present the profiles extracted from artificial downsized images convolved with the JWST F356W PSF, indicated by dashed curves, and present the deconvolved profiles, shown as solid curves. The resolution of the artificial image is indicated by the ratio of galaxy half-light radius (R₅₀) to PSF FWHM, denoted at the top of the panel. The arrow denotes the disk break seen in the intrinsic profile.