  This paper describes an N-body model for the dynamical evolution of the
nearby globular cluster M4. The initial conditions, with N = 484710 particles,
were generated from a published study of this cluster with a Monte Carlo code.
With the Monte Carlo code, these initial conditions led, after 12 Gyr of
dynamical and stellar evolution, to a model which resembles M4 in terms of its
surface brightness and velocity dispersion profiles, and its local luminosity
function. Though the N-body model reported here is marred by some errors, its
evolution can be compared with that of the published Monte Carlo model, with a
result from the synthetic evolution code EMACSS, and with M4 itself.
