160260 andCGCG 97087.
Some objects have individual positional errors up to .
Therefore MIR images have been re-centered on the optical ones. It is thus not possible to analyze their MIR surface brightness distribution in any detail. Images in the LW2 filter are marginally more extended than the LW3 ones. The MIR emission is generally peaked at the center and decreases smoothly throughout the disk. However CGCG 97087, CGCG 160088 and CGCG 160095 show an extended IR emission and some structure.