  In this note we propose that recently discovered radio pulsar J0250+5854 with
23.5 sec spin period is presently at the Hall attractor stage. This can explain
low temperature and absence of magnetar-like activity of this source together
with its spin period and period derivative. We present results of calculations
of the evolution of this source in a simple model of magnetic field decay. The
neutron star could start its evolution as a magnetar with initial field $\sim
10^{14}-10^{15}$ G for realistic range of parameter $Q$ describing crust
imperfections. Future measurements of surface temperature and age of this
neutron star might help to probe this hypothesis.
