  In this work, we have considered the recently proposed new Tsallis Agegraphic
Dark Energy model (NTADE) (Mod. Phys. Lett. A 34, 1950086, 2019) within the
framework of a flat Friedmann-Robertson-Walker(FRW)
  Universe by taking various values of the parameter $\delta$. The NTADE model
shows the current phase transition of the Universe from
  decelerated to accelerated phase. The NTADE EoS parameter shows a rich
behaviour as it can be quintessence-like or phantom-like depending on the value
of $\delta$. For discriminating the NTADE model from $\Lambda$CDM, we have
plotted the statefinder parameters $r(z)$, $s(z)$ and $(r, s)$, $(r, q)$ pair.
The NTADE model shows distinct evolutionary trajectories of their evolution in
($ r, s$) and ($ r, q$) plane. An analysis using the snap parameter and
  the $\omega_{D}-\omega_{D}^{'}$ pair dynamical analysis have also been
performed.
