We present parsec-scale (~2 pc) JWST NIRCam/MIRI observations for the Evil Eye Galaxy, M64. M64 is a post minor merger galaxy, features a dusty, compact, inner disk. Located at a distance of 4.4 Mpc, this galaxy serves as an ideal case for resolving massive star clusters and HII regions. We present new continuum-subtracted Pa-alpha, Br-alpha, and 3.3 um PAHs images from NIRCam and another PAHs emissions and dust from MIRI observations. The Pa-alpha and Br-alpha images reveal resolved HII regions and complex stellar feedback features in M64, with corresponding structures also found in PAHs maps. We identify resolved young star clusters and HII regions and estimate their characteristics (e.g., sizes and morphologies). We also discuss the interaction between star cluster/HII regions and the surrounding medium.
