Abstract We present measurements of morphological parameters from fitting 53,885 galaxies detected to a magnitude limit of F356W 2.5), the color gradients are nearly flat with no dependence on mass, indicating that the stellar populations are more uniform throughout. The structural measurements presented are accurate to 20% or better for most galaxies with F356W < 27.0 mag and will enable further studies of galaxy morphology to z ∼ 10.
McGrath et al. (2026) studied this question.