That depends what we mean by "dark matter". Do you mean all the matter that we can't see? Clearly there's plenty of that in brown dwarfs, black holes, dim stars, faraway stars, faraway galaxies, and all sorts of other things. But what is usually meant by dark matter - a particular component of the universe - is almost certainly non-baryonic. When we talk about dark matter (and when I talk about dark matter), I'm referring to the stuff that flattens galactic rotation curves, and especially important, the stuff that provides gravitational potential wells for galaxies to form in - before brown dwarfs and the rest even exist. Almost certainly baryonic, and not in the form of brown dwarfs or black holes.