  We use the M{\o}ller and Landau-Lifshitz energy-momentum definitions in
General Relativity (GR) to evaluate the energy-momentum distribution of the
phantom black hole space-time. The phantom black hole model was applied to the
supermassive black hole at the Galactic Centre. We obtain that in both
pseudotensorial prescriptions the energy distribution depends on the mass $M$
of the black hole, the phantom constant $p$ and the radial coordinate $r$.
Further, all the calculated momenta are found to be zero. The limiting cases
$r\rightarrow 0$, $r\rightarrow \infty $ and $r\rightarrow -\infty $ have also
been the subject of the study.
