Nonparametric morphological parameters for our sample of 14 unique massive quiescent galaxies for the F200W NIRCam filter. Top: ﹩{\mathrm{log}}_{10}(A)﹩ (asymmetry) vs. concentration, C. The merger line was taken from C. J. Conselice (2003), and the disk–intermediate and intermediate–elliptical boundaries were implemented following M. A. Bershady et al. (2000). Bottom: Gini coefficient vs. M₂₀. The boundary lines were implemented following J. M. Lotz et al. (2008).