  We report the results of the {\it Chandra} ACIS-S observations of the
elliptical galaxy NGC 821, which harbors a supermassive nuclear black hole (of
$3.5 \times 10^7 M_{\odot}$), but does not show sign of AGN activity. A small,
8.5$^{\prime\prime}$ long ($\sim 1$ kpc at the galaxy's distance of 23 Mpc),
S-shaped, jet-like feature centered on the nucleus is detected in the 38 ksec
ACIS-S integrated exposure of this region. The luminosity of this feature is
$L_X \sim 2.6 \times 10^{39} \rm ergs s^{-1}$ (0.3-10 keV), and its spectrum is
hard (described by a power-law of $\Gamma = 1.8^{+0.7}_{-0.6}$; or by thermal
emission with $kT >2$ keV). We discuss two possibilities for the origin of this
feature: (1) a low-luminosity X-ray jet, or (2) a hot shocked gas. In either
case, it is a clear indication of nuclear activity, detectable only in the
X-ray band. Steady spherical accretion of the mass losses from the central
stellar cusp within the accretion radius, when coupled to a high radiative
efficiency, already provides a power source exceeding the observed radiative
losses from the nuclear region.
