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Globular cluster in the constellation Libra
NGC 5897
The globular cluster NGC 5897 imaged with an amateur telescope.
The stars of the cluster have only 0.91% of the Sun's metallicity, while the abundance of elements produced by the alpha process is roughly 5 times larger. This means that the cluster formed in a time before the galaxy formed a disk and spiral arms. However, some of the stars are apparently younger, indicating multiple star-forming epochs.
NGC 5897 has a diameter of 12.6 arcminutes and an apparent magnitude of 8.5.
References
Shapley, Harlow; Sawyer, Helen B. (August 1927), "A Classification of Globular Clusters", Harvard College Observatory Bulletin, 849 (849): 11–14, Bibcode:1927BHarO.849...11S.