We consider, in Palatini formalism, a modified gravity of which the scalar field derivative couples to Einstein tensor. In this scenario, Ricci scalar, Ricci tensor and Einstein tensor are functions of connection field. As a result, the connection field gives rise to relation, hµν = f gµν between effective metric, hµν and the usual metric gµν where f = 1 − κφ ,α φ,α/2. In FLRW universe, NMDC coupling constant is limited in a range of −2/φ 2 < κ ≤ ∞ preserving Lorentz signature of the effective metric. Slowly-rolling regime provides κ < 0 forbidding graviton from travelling at superluminal speed. Effective gravitational coupling and entropy of blackhole's apparent horizon are derived. In case of negative coupling, acceleration could happen even with w eff > −1/3. Power-law potentials of chaotic inflation are considered. For V ∝ φ 2 and V ∝ φ 4 , it is possible to obtain tensor-to-scalar ratio lower than that of GR so that it satisfies r < 0.12 as constrained by Planck 2015 [35]. The V ∝ φ 2 case yields acceptable range of spectrum index and r values. The quartic potential's spectrum index is disfavored by the Planck results. Viable range of κ for V ∝ φ 2 case lies in positive region, resulting in less blackhole's entropy, superluminal metric, more amount of inflation, avoidance of super-Planckian field initial value and stronger gravitational constant. *