We study stationary relativistic scattering theory for a ␦-sphere interaction formally given by the Hamiltonian HϭH D ϩ␣␦(͉x គ ͉ϪR), x គ R 3 , ␣R, RϾ0 with the boundary conditions of second type. First we give the mathematical definition of the model, self-adjointness of the Hamiltonian, indicial equation, stationary scattering theory and the spectral properties. Next we extend the model by adding a Coulomb potential and provide useful mathematical definitions and corresponding stationary scattering elements.