Examples of galaxies in the EGS images, with the Sérsic index increasing from the top to bottom rows (disc to spheroid morphology) and the redshift increasing (from z ≈ 0 to 2) from the left to right columns. The filters have been selected to have the similar rest-frame optical wavelength. The measured structural parameters (n, C, G, M₂₀) are also listed in each panel. The galaxies on the right two columns are also observed in CEERS, which are shown in the left two columns of Fig. 6.