We have started multi-color imaging program of nearby galaxies since last year and present preliminary result here. We selected 12 nearby galaxies classfied from E to Sab type and observed in BVRIJHK' bands. Photomtric parameters such as isophotal diameter, axial ratio, isophotal magnitude were measured and observed colors were compared with theoritical model. We find a standard evolution model agrees well with observed results.

• KENSHl YANAGISAWA(Department of Astronomy, School of Science, the University of Tokyo)
• NOBUNARI ITOH(Department of Astronomy, School of Science, the University of Tokyo)
• TAKASHI ICHIKAWA(Kiso Observatory, Institute of Astronomy, the University of Tokyo)