We have an ongoing program with the 2.56m Nordic Optical Telescope on La Pa
lms to take very deep, subarcsecond optical images of all the blazars detec
ted by the EGRET experiment onboard the GRO-satellite and of a comparison s
ample of blazars that EGRET has observed BUT NOT detected. Our goal is to s
tudy the host galaxy properties and the close blazar neighbourhood in both
samples in order to search for possible differencies among their morphologi
cal and environmental properties. First preliminary results of this program
are shown.