We consider disformal transformations in a subclass of Horndeski theory in which a scalar field is kinetically coupled to Einstein tensor. We apply a disformal transformation on a seed hairy black hole solution of this theory and we show that there is a transition of a black hole to a wormhole. We also show that the null energy condition is violated in the wormhole configuration and we study the stability of the wormhole solution by calculating the time evolution of scalar perturbations in this geometry. Contents I. Introduction 1 II. Black Hole Solution with a Scalar Field Kinetically Coupled to Einstein Tensor 2 III. Generating a wormhole solution by a disformal transformation 4 IV. Testing of the energy conditions 6 V. Evolution of scalar perturbations on the wormhole geometry 8 A. Two-Way Wormhole 9 B. One-way Wormhole 10 VI. Conclusions 11 A. Appendix 12 References 13