  The proposal of pilgrim dark energy is based on the speculation that
phantom-like dark energy possesses enough resistive force to preclude the black
hole formation in the later universe. We explore this phenomenon by assuming
the generalized ghost version of pilgrim dark energy. We find that most of the
values of the interacting ($\xi^2$) as well as pilgrim dark energy ($u$)
parameters push the equation of state parameter towards phantom region. The
squared speed of sound shows that this model remains stable in most of the
cases of $\xi^2$ and $u$. We also develop $\omega_\Lambda-\omega'_\Lambda$
plane and observe that this model corresponds to thawing as well as freezing
regions. Finally, it is shown that the non-interacting and interacting
generalized ghost versions of pilgrim dark energy correspond to $\Lambda$CDM
limit on the statefinder plane.
