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This paper reports on a study of the morphological characteristics of several samples of galaxies drawn from the 1401 objects which comprise the Second Byurakan Survey (SBS). These samples have been chosen to provide information for studies of the relation between galaxy interactions and galaxy star formation activity. Our samples include 110 SBS galaxies in 107 mergers, 58 SBS galaxies in 47 interacting systems, and 49 SBS galaxies in 30 close pairs (projected separations DD 50 kpc and radialdoi:10.1086/339980 fatcat:em5rjkexbrfrzakbugsglr7lme