There are three separate concepts:
a body which absorbs all incident radiation
a body which is in a state of internal thermal equilibrium
a body which is in a state of internal thermal equilibrium, and also in equilibrium with its surroundings, which have a well-defined temperature
A black body is one which obeys 1. Such a body does not have to be in a state of internal thermal equilibrium, but if it is then it will emit black body radiation at the temperature $T$ of the body.
If a black body is in close to a state of internal thermal equilibrium but in surroundings which are either not in equilibrium or are at some other temperature, then the emission from the black body will include a part $\rho_T$ which is thermal, and another part which depends on the surroundings. Such a body is not in a true equilibrium, even internally, but it may be that the surroundings are only having a slow effect on it, so its state is moving quasistatically from one equilibrium state to another. If so then one may say it is well-approximated by an internal equilibrium and therefore it is emitting black body radiation.
Finally, if a black body is in equilibrium with surroundings at the same temperature, then the absorption and emission will agree in full and in detail.