  In this paper, we search for correlations between the intrinsic properties of
galaxies and the Bose-Einstein condensate (BEC) under a scalar field dark
matter (SFDM) at temperature of condensation greater than zero. According to
this paradigm the BEC is distributed in several states. Based on the galactic
rotation curves collected in SPARC dataset, we observe that SFDM parameters
present a weak correlation with most of the galaxy properties, having only a
correlation with those related to neutral hydrogen emissions. In addition, we
found evidence to support of self-interaction between the different BEC states,
proposing that in future studies must be considered crossed terms in SFDM
equations. Finally, we find a null correlation with galaxy distances giving
support to non-hierarchy of SFDM formation.
