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The limiting unabsorbed flux in the core is $f_x$ (0.5$-$6.0 keV) $\\simeq$ 3 $\\times$ 10$^{-16}$ erg s$^{-1}$ cm$^{-2}$ ($L_X$ $\\simeq$ 1 $\\times$ 10$^{30}$ erg s$^{-1}$ at 5.2 kpc). We estimate that ~$60\\pm 20$ of these are cluster members, of which ~30 lie within the core ($r_c$ $=$ 155 arcsec), and another ~30 between 1$-$2 core radii. We identify four new optical counterparts, for a total of 45 likely identifications. 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