  In this work, we construct galactic halos in order to fit the rotation curves
(RCs) of a sample of low surface brightness (LSB) galaxies. These halos are
made of Fuzzy Dark Matter (FDM) with a multimode expansion of non-spherical
modes that in average contribute to the appropriate density profile consisting
of a core and an envelope needed to fit the rotation curves. These halos are
constructed assuming a solitonic core at the center and two types of envelopes,
Navarro-Frenk-White and Pseudo-Isothermal density profiles. The resulting FDM
configurations are then evolved in order to show how the average density
changes in time due to the secular dynamical evolution, along with a
condensation process that lead to the growth of the solitonic core.
