  We report kinematic and thermal signatures associated with the directly
imaged protoplanet candidate in the Elias 2-24 disc. Using the DSHARP ALMA
observations of the $^{12}$CO J=2-1 line, we show that the disc kinematics are
perturbed, with a detached CO emission spot at the location of the planet
candidate and traces of spiral wakes, and also that the observed CO emission
intensities require local heating. While the foreground extinction hides the
velocity channels associated with the planet, preventing a planet mass
estimate, the level of gas heating implied by the CO emission indicates the
presence of a warm, embedded giant planet. Comparison with models show this
could either be a $\gtrsim 5$M$_\mathrm{Jup}$, or a lower mass ( $\gtrsim
2$M$_\mathrm{Jup}$) but accreting proto-planet.
