M67 (NGC 2682) is a dynamically evolved old (4 Gyr) open cluster in the Milky Way. Due to its nearness and relatively low levels of dust in the line-of-sight, it has been extensively observed both in surveys and targeted observations. We perform new N-body simulations of M67 using the updated nbody6++gpu and also compare these models to observational data from the Gaia survey. While overall cluster parameters such as mass and main-sequence turnoff mass match observations, further simulations are needed to better match the blue straggler population. Further work is needed to investigate the binary transient systems in the models.
