  NMDC-Palatini cosmology in slow-roll regime is of our interests. We present
flat FLRW cosmological NMDC-Palatini field equations and acceleration
condition. Late time trajectory is approximated. Chaotic inflation potential is
considered here as it is viable in a range of positive coupling constant as
constrained by CMB results. Phase portraits show that the NMDC-Palatini gives
new saddle-point solutions. In $V \propto \phi^2$ potential, the NMDC-Palatini
effect enlarges the acceleration-allowed region from that of GR case.
