In this paper I provide a general framework based on δN formalism to study the features of unavoidable higher dimensional non-renormalizable Kähler operators for N = 1 supergravity (SUGRA) during primordial inflation from the combined constraint on nonGaussianity, sound speed and CMB dipolar asymmetry as obtained from the recent Planck data. In particular I study the nonlinear evolution of cosmological perturbations on large scales which enables us to compute the curvature perturbation, ζ, without solving the exact perturbed field equations. Further I compute the non-Gaussian parameters f N L , τ N L and g N L for local type of non-Gaussianities and CMB dipolar asymmetry parameter, A CM B , using the δN formalism for a generic class of sub-Planckian models induced by the Hubbleinduced corrections for a minimal supersymmetric D-flat direction where inflation occurs at the point of inflection within the visible sector. Hence by using multi parameter scan I constrain the non-minimal couplings appearing in non-renormalizable Kähler operators within, O(1), for the speed of sound, 0.02 ≤ c s ≤ 1, and tensor to scalar, 10 −22 ≤ r ⋆ ≤ 0.12. Finally applying all of these constraints I will fix the lower as well as the upper bound of the non-Gaussian parameters within,and O(17.4 − 34.7) ≤ g N L ≤ 648.2, and CMB dipolar asymmetry parameter within the range, 0.05 ≤ A CM B ≤ 0.09.