The galaxy presents as a moderately luminous object at a redshift of approximately 0.24. Morphologically, the galaxy appears to be in the late stages of a merger event. The core is bright and elongated with distinct, bright nodes suggesting interacting galactic nuclei. There is some disturbance in the surrounding morphology and the edges are fairly indistinct, which is consistent with ongoing tidal interactions and gravitational disturbances, with signs of minor star formation activity. The galaxy exhibits a generally smooth appearance despite the merger, with an overall roundness but with some features suggestive of a flattened spheroidal or disk-like component.
