  We presented timing results of PSR B2035+36 using ~9-yr observations with the
Nanshan 25-m radio telescope. PSR B2035+36 was reported to exhibit significant
changes in pulse profile correlated with spin-down state variations. We found
that the pulsar underwent a glitch with a jump in the frequency of
$\Delta{\nu}\sim12.4(5)\, \rm nHz$ around MJD 52950. Unusually, the spin-down
rate increased persistently over $800$ days after the glitch, and the average
spin-down rate of post-glitch was about $9.6\%$ larger than pre-glitch.
Accompanied with the glitch activity, pulse profile became narrower. The pulsar
began to switch between two emission modes after the glitch, with pulse width
($W_{\ 50 \rm mean}$) of $8.5(7)^{\circ}$ and $3.7(3)^{\circ}$, respectively.
Besides that, the relatively narrow pulse profile gradually became dominant.
All of the observations indicate that there should be connection between
magnetospheric behavior and glitch activity. We discuss one possibility of
magnetosphere fluctuation triggered by glitch event.
