M71, A Globular Cluster, - this image cropped and reduced from the original photo, Click on photo above for a full resolution image.
This doesn't look like a typical globular cluster, and for a long time, the classification of M71 as a globular was uncertain. Many astronomers thought it was a rather condensed open cluster similar to M11, whereas others thought it was more like the loose globular M68. Evidence to assign it one way or another was conflicting. Nevertheless, there's now consensus that M71 is a loose globular. It is 13,000 light years distant with the majority of the stars within a  27 light year diameter, small for a globular cluster. However, as an indication of just how loose and diffuse it is, faint members have been detected out to a diameter of  90 light years.

This globular cluster is fairly easy to find and fairly easy to see with binoculars. It is located high in the summer's Milky Way, north of Altair, about 1/3rd of the way to Deneb. Six inch or larger telescopes are required to resolve it into stars, some of which can be resolved all the way to the center. It contains maybe 30 bright stars scattered over a field of 7.8 arc minutes, with an overall surface brightness of magnitude 8.2.

11" Celestron HDEdge, F10, moddifiied Schmidt Cassegrain Telescope, Canon Ra camera, placed at the scope's prime focus
9 photos aligned and averaged together, then brightness, color, and contrast enhanced.
Each photo, 40 seconds exposure at ISO 3200