  We have presented the first joint {\it XMM-Newton} and {\it NuSTAR} analysis
of the millisecond pulsar (MSP) binary PSR J1653$-$0158. The 75-minute orbital
period inferred from optical and gamma-ray observations together with the
1.97-ms pulsation in the gamma-rays indicate that this system is the most
compact Black Widow MSP system known to date. The orbital period was not
detected in the {\it XMM-Newton} and {\it NuSTAR} data, probably due to
insufficient photon counts obtained in the observations. Fitting the joint
X-ray spectrum of PSR J1653$-$0158 with a power law gives a photon index
$\Gamma = 1.71 \pm 0.09$. The X-ray luminosity of the source in the
($0.2-40$)~keV band is deduced to be $1.18 \times 10^{31}\;\!{\rm erg~s}^{-1}$,
for an adopted distance of 0.84~kpc. We have shown that the broad-band X-ray
spectrum can be explained by synchrotron radiation from electrons accelerated
in the intra-binary shock, and the gamma-rays detected in the {\it Fermi} data
are curvature radiations from electrons and positrons in the pulsar
magnetosphere. Our kinematic analysis of the Tidarren systems PSR~J1653--0158
and PSR~J1311--3430 indicates that the two Tidarren systems are likely to have
originated in the Galactic Disk.
