DM profiles of a 10¹⁰ M_⊙ halo at z = 0 for different values of m₂₂ as in Safarzadeh & Spergel (2020). The dashed lines show the central solitonic profiles. The blue line shows the NFW profile of a 10¹⁰ M_⊙ halo at z = 0. The solid lines show our model for the full halo profile, which is a combination of the FDM profile transitioning to an NFW profile, described by Equations (12) and (13). The vertical lines indicate the size of the FDM core radius. The green solid line corresponds to the typical stellar density profile for this halo mass, extracted from the TNG50.