The IRAS Point Source Catalog shows an object called IRAS19321+2757 with 4 other associated objects:
AFGL 2417 .... Object 2417 in the Air Force Geophysical Labs catalog IRC +30374 .... CalTech's 'Infrared Catalog ' V1129 Cygni .... Variable star number 1129 in Cygnus NSV 12165 .... 'Suspected Variable' star number 12165The way that the IRAS catalog works is that all objects listed in up to 35 other catalogs within 5 arcminutes or so of the IRAS sky position are listed as possible candidates for the infrared object. This doesn't mean they are related to each other, especially in crowded regions of the sky where lots of unrelated objects can be in the same sky patch.
I looked at the literature for AFGL 2417. It was studied by Terry Jones and his co-workers at the University of Minnesota over 9 years and found to be a variable star with a period of 625 days. This doesn't match the period of V1129 Cygni ( 270.5 days) which many thought was the optical candidate for the infrared star, and is actually 4 arcminutes away from the position of AFGL 2417 also suggesting not a good match. Jones et al. identify this infrared object, and many others in the AFGL survey, as a carbon-type red giant with a luminosity about 1000 times that of the sun, but it is so enveloped by its own dusty cloud of gas that it is optically very faint. For more information, have a look at the journal 'Astrophysics Journal Supplement, volumn 74, page 785.