  We investigate the ferromagnetic (spin polarization) condensation in (2+1)
flavor Nambu Jona-Lasinio(NJL) model with non-zero current quark masses at
finite temperature and density which may be relevant in the context of neutron
stars. The spin polarization condensation arises due to a tensor type
interaction which may be generated due to non-perturbative effects in Quantum
Chromodynamics(QCD). In this investigation we have shown the interplay between
chiral condensate and spin polarization condensation for different values of
tensor coupling. Spin polarization in the case of 2+1 flavor is different from
two flavor case because of additional F$_8$ condensate associated with
$\lambda_8^f$ flavor generator. We find a non-zero value of the two spin
condensates in the chirally restored phase. Beyond a certain temperature the
spin polarization condensates vanish for rather large quark chemical
potentials. The spin condensates affect the chiral phase transition, quark
masses, and the quark dispersion relation. The spin polarization condensate
appears only in the chiral restored phase for light quarks. For large enough
tensor couplings, it is observed that the spin polarization condensate acts as
a catalyst for chiral symmetry restoration. Thermodynamic behavior of $F_3$ and
$F_8$ are found to be different and they affect the quark masses differently.
