J   K_S CMD of the simulated nuclear clusters after 13 Gyr of evolution for a distance of 8 kpc to the GC and an average reddening of mag. The different stellar generations that were added to the simulations can clearly be distinguished in the CMD. Stars marked in red have K_S < 18.5 and are used for comparison with the density profile of resolved stars from Gallego Cano et al. (2018). The remaining stars are used to create the diffuse light profile of the simulated clusters.