The topic of to what extent are gravitational waves just like any other wave (such as electromagnetic) seems a little complicated to answer. In Einstein's field equations
G_{\mu \nu} = \frac{8 \pi G}{c^4} T_{\mu \nu}
the left side includes geometric stuff--the metric and its derivatives--and the right side includes ordinary non-gravitational matter, energy and momentum. So the electromagnetic field carries energy and momentum, so it makes an appearance on the right side, as a contribution to T_{\mu \nu}. A gravitational wave, however, is a fluctuation of the metric tensor, and so it would appear on the left side, as a contribution to G_{\mu \nu}. So in this standard form for General Relativity, it's not at all obvious that a gravitational wave should behave like any other wave under the influence of gravity.
But perhaps the fact that gravitational waves are treated in GR the same as other waves is more apparent in the spin-2 field theory approach to gravity. In this approach, you start with linearized gravity, which describes perturbations h_{\mu \nu} to the flat spacetime metric \eta_{\mu \nu} via a wave equation that uses stress-energy, t_{\mu \nu} as a source. To get to something equivalent to GR, the source t_{\mu \nu} has to include not only the energy/momentum due to nongravitational fields, but also the stress-energy due to h_{\mu \nu} itself. So in this way of formulating gravity, it is maybe clearer that propagating perturbations to the metric act just like any other wave when it comes to gravity.