Recent DSN and DSN/WET campaigns have identified 19 probable pulsation modes in the delta Scuti star FG Vir. We evolve and pulsationally analyze the 1.8-2.0msun models of FG Vir trying to match the observed frequencies. In general, our evolutionary models and mode identifications agree well with those of Breger et al. (1995) for the 10 modes reported from the 1993 campaign. However, our models have difficulty matching all 9 additional preliminary frequencies determined in the 1995 campaign.