  We select 456 gas-star kinematically misaligned galaxies from the internal
Product Launch-10 of MaNGA survey, including 74 star-forming (SF), 136
green-valley (GV) and 206 quiescent (QS) galaxies. We find that the
distributions of difference between gas and star position angles for galaxies
have three local peaks at $\sim0^{\circ}$, $90^{\circ}$, $180^{\circ}$. The
fraction of misaligned galaxies peaks at $\log(M_*/M_{\odot})\sim10.5$ and
declines to both low and high mass end. This fraction decreases monotonically
with increasing SFR and sSFR. We compare the global parameters including gas
kinematic asymmetry $V_{\mathrm{asym}}$, HI detection rate and mass fraction of
molecular gas, effective radius $R_e$, S\'{e}rsic index $n$ as well as spin
parameter $\lambda_{R_e}$ between misaligned galaxies and their control
samples. We find that the misaligned galaxies have lower HI detection rate and
molecular gas mass fraction, smaller size, higher S\'{e}rsic index and lower
spin parameters than their control samples. The SF and GV misaligned galaxies
are more asymmetric in gas velocity fields than their controls. These
observational evidences point to the gas accretion scenario followed by angular
momentum redistribution from gas-gas collision, leading to gas inflow and
central star formation for the SF and GV misaligned galaxies. We propose three
possible origins of the misaligned QS galaxies: (1) external gas accretion; (2)
merger; (3) GV misaligned galaxies evolve into QS galaxies.
