The galaxy presents as a disturbed system, likely undergoing a significant merger event. Two prominent, relatively compact, and bright nuclei are observed, suggesting two galaxies in close proximity, interacting gravitationally. The overall morphology is complex and lacks a clear, well-defined structure. There's evidence of tidal features, potentially faint streams or tails of material extending from the central regions of the galaxy, though image quality limits detailed characterization. The central region exhibits a yellowish-green hue, possibly indicative of an older stellar population or dust obscuration. The outskirts appear somewhat redder. There does not appear to be a high rate of star formation or presence of young stars. The galaxy is approximately 9 kpc in radius and is located at a redshift of approximately 0.3, indicating it's at a significant cosmological distance.
