If there was, it would have been observed by now through observations of binary systems. Don't forget that galactic clusters also show evidence of dark matter too, so the deviations from classical expectations do work on a large scale. It's also worth remembering that one aspect of the composition of dark matter is already known: the neutrino. Unfortunately, they only form a relatively small portion of the total amount that has been speculated and the robustness of the Standard Model doesn't offer any suggestions as to what the rest can realistically be.