[2] In total there are 41 galaxies which are confirmed to be members of the cluster.
[1] The cluster is classified as a Bautz-Morgan type III and Rood-Sastry class F cluster, indicating morphological irregularity and perhaps dynamical youth.
[4] It is receding from the Milky Way galaxy with a velocity of 12385 km/s.
[2] Abell 2152 is the nearest cluster in which significant gravitational lensing of a background source has been observed.
The arc-like background galaxy, known as J160529.52+162633.9, lies at a redshift z=0.1423 and has been magnified by a factor ~1.9 due to the lensing effect.