It depends.
As you mentioned, there is no stress tensor for the gravitational field. Hence, we can't localize gravitational energy. In this specific sense, it is common to say there is no gravitational energy. I should add that you can define pseudotensors.
Globally, however, you can define notions of energy that comprise both matter and gravitational contributions. There are a few different notions that may or not coincide depending on the specific problem you're interested in (for example, some of them might change with time, while others are conserved). They are the Komar mass the ADM mass, and the Bondi–Sachs mass. At least some of these definitions require asymptotically flat or stationary spacetimes and they are all discussed in Wikipedia. I am unaware of any definition that encompasses all spacetimes (and that would likely be meaningless anyway, since a constant cosmological constant would be expected to lead to a diverging energy in a spacetime that is not spatially compact).