  Many dark energy (DE) models have been proposed, in recent years, to explain
acceleration of the Universe expansion. It seems necessary to discriminate the
various DE models in order to check the viability of each model. Statefinder
diagnostic is a useful method which can differentiate various DE models. In
this paper, we investigate the statefinder diagnosis parameters for the
holographic dark energy (HDE) model in two cosmological setup. First, we study
statefinder diagnosis for HDE in the context of flat Friedmann-Robertson-Walker
(FRW) Universe in Einstein gravity. Then, we extend our study to the DGP
braneworld framework. As system's IR cutoff we chose the Hubble radius and the
Granda-Oliveros cutoff inspired by Ricci scalar curvature. We plot the
evolution of statefinder parameres $\{r,s\}$ in terms of the redshift parameter
$z$. We also compare the results with those obtained for statefinder diagnosis
parameters of other DE models, in particular with $\Lambda$CDM model.
