  In this paper, we study the charged and uncharged BTZ counterpart of the
Black-Bounce proposed by Simpson and Visser recently. For the uncharged case,
we find that the temperature is not modified by the bounce parameter. We also
find that the wormhole side of the solution must always be supported by exotic
matter over the throat. For the charged case we find that the thermodynamics is
changed and the bounce parameter controls a phase transition, affecting the
sign of the heat capacity and therefore the stability of the system. For the
uncharged case, we find that there are no stable orbits for both massive and
massless incoming particles while stable orbits are present for the charged
case and the bounce parameter affects the points of stability.
