We are pursuing a variety of avenues in our study of the evolution of galaxy properties. In terms of morphological evolution (including internal kinematics) we have been studying E+A galaxies and have shown that these are transitional types between gas-rich (presumably spirals) and gas-poor, pressure supported systems (ellipticals). In terms of understanding the role of environment in determining star formation rates, we have been obtaining Halpha measurements of cluster galaxies out to z ~ 0.8. In terms of understanding the evolution of galaxies in color-magnitude space, we have been examining the developement of the red sequence of galaxies. For more details, see papers 23, 43, 46, 60, 62, 70, 74, 78, and 84 in the publication list.