  We demonstrate in this paper the use of asymmetry in conjunction with the
integrated (B-V) color of galaxies for physical morphological purposes. We show
how color-asymmetry diagrams can be used to distinguish between various types
of galaxies, including ellipticals, late and early type disks, irregulars and
interacting/merging galaxies. We also show how asymmetry can be used to help
decipher the morphology of nearby starbursts, and galaxies in the Hubble Deep
Field.
