  We employ the quark part of the symmetric energy-momentum tensor current to
calculate the transition gravitational form factors of the $N(1535) \rightarrow
N$ by means of the light cone QCD sum rule formalism. In numerical analysis, we
use two different sets of the shape parameters in the distribution amplitudes
of the $ N(1535) $ baryon and the general form of the nucleon's interpolating
current. It is seen that the momentum squared dependence of the gravitational
form factors can be well described by the p-pole fit function. The results
obtained by using two sets of parameters are found to be quite different from
each other and the $N(1535) \rightarrow N$ transition gravitational form
factors depend highly on the shape parameters of the distribution amplitudes of
the $N(1535)$ state that parametrize relative orbital angular momentum of the
constituent quarks.
