  The problem of the possibility of observing a uniform sky glow through the
throat of a Morris--Thorne wormhole by an observer located in another
asymptotically flat space-time is considered. It is shown that an individual
star has multiple images, and the image of a luminous sky has a complex
structure and contains ring structures. The reasons for the emergence of such
structures are considered. The distribution of radiation intensity in the image
along the radial coordinate is constructed.In addition, an image of the
Morris-Thorne wormhole was constructed against the background of uniform sky
radiation in the observer's space. A comparison to observations can be made by
producing a synthetic Morris-Thorne type wormhole image against a CMB
background. This image has been constructed by a combination of the images for
inner and outer areas.
