  We have applied isovector and isoscalar tensor current to evaluate the tensor
form factors of the $ N(1535) \rightarrow N $ transition with the help of the
light-cone QCD sum rule method. In numerical computations, have used the most
general forms of the interpolating current for the nucleon and the tensor
current together with two different sets of the input parameters in the DAs of
the $N(1535)$ state. We have obtained that the values of $N(1535) \rightarrow
N$ transition tensor form factors very sensitive to the input parameters of the
distribution amplitudes of the $N(1535)$ state. We have acquired that the $Q^2$
dependence of $N(1535) \rightarrow$ transition tensor form factors is well
defined by a p-pole fit function.
