a flux density of 51.4$\pm$4$\mu$Jy. Since the 24$\mu$m flux would be dominated by redshifted hot dust and polycyclic aromatic hydrocarbon emission, it indicates the presence of dust within the galaxy. The age-extinction degeneracy is very well known for red galaxies. Most recently, @Stern:06 have shown that the optical/near-infrared photometry of dusty, extremely red objects (EROs) is almost identical to that of evolved, passive EROs, and that only the detection of reprocessed emission at mid- and far-infrared wavelengths can break the degeneracy. Nevertheless, Mobasher et al. (2006) suggest that the 24$\mu$m emission could be explained by the presence of an obscured active nucleus. While this is possible, at $z\sim6.5$, the [*Chandra*]{} 2$-$8 keV band traces 15$-$60 keV emission, energies which are relatively immune to absorption. The $Chandra$ detection limit corresponds to L$_{\rm X}$ of 3$\times$10$^{43}$ erg s$^{-1}$ at $z=6.5$ while the mid-infrared detection implies $\nu$L$_{\nu}$ at rest 3[$\mu$m]{} of 3$\times$10$^{45}$ erg s$^{-1}$. The 10[$\mu$m]{}  to X-ray luminosity ratios of local Seyfert nuclei are $\sim$3 [e.g. @Krabbe], and the flat spectrum of Seyferts in $\nu L_{\nu}$, implies that either large (N$_{\rm H}>>10^{24}$cm$^{-2}$) column densities of neutral gas must be obscuring the hard X-ray emission or the active galactic nucleus (AGN) is an 