The cluster is located at z = 0.1582,[3] and is X-ray luminous (LX = 7.1 × 1044 erg s−1),[4] containing a mild intracluster medium temperature of 7.1 keV.

Indian astronomers from Savitribai Phule Pune University noticed a burst of radio jet activity, from its central black hole.

Led by Surajit Paul, he mentioned the first pair of radio lobes discovered are the oldest he and the astronomers had seen.

[9] Following the primary pair of radio lobes to 2MASX J10222849+5006200, another team of astronomers led by Gopal-Krishna, found the galaxy has drifted to the central region of the cluster by 250,000 light-years from its original position.

Here, the galaxy erupted again by going through a new active phrase; it created another set of radio lobes, this time younger.