In addition to what's said above, it should be pointed out that Newtonian gravitation does predict bending of light around massive bodies after making a some very reasonable assumptions. Basically, rather than being combined into the standard force law, you should think of Newtonian gravity as a field equation: ##\vec{E} = GM/r^2## along with a force law analogous to the electrostatic force, ##\vec{F} = m\vec{E}##. Now, despite not knowing how, exactly, such a gravitational field affects massless objects, it's fairly clear that if massless objects exist it must affect them. Just start with a massive object and apply these equations plus ##\vec{F}=ma## and deduce that it accelerates at a rate independent of its mass, ##\vec{a} = \vec{E}##. Now take the limit of the mass to zero and the acceleration stays the same. You can make the mass infinitesimally small and it will still accelerate at the same rate. It would be exceedingly strange if gravitational acceleration were discontinuous—zero for something massless and finitely small for anything arbitrarily close—so it's reasonable to deduce that the identification of acceleration with the gravitational field is completely general. Then by treating light as massless particles, you can figure out how much it deflects when passing by massive bodies. This was done around 1800 and generally accepted by the scientific community, well before Einstein and relativity.
It's commonly stated that, as Eddington tested, GR predicts light bends and Newtonian gravity predicts it does not. This is not true, or at least doesn't reflect the understanding of Newtonian gravity at the time. In fact, the prediction by GR is that light bends exactly twice as much as Newtonian gravity predicts. It's also now generally accepted that the accuracy of Eddington's experiment was insufficient to support his conclusion in favour of GR; however, since then we've done much more precise tests that have confirmed relativity's prediction over Newton's.