The galaxy appears to be in the process of merging with another galaxy. Evident are two distinct, rounded concentrations of light, presumably the galactic cores, exhibiting a redder hue. These redder cores are indicative of older stellar populations, potentially with ongoing or recent star formation in the central regions, possibly due to the tidal effects of the ongoing interaction. A more diffuse, greenish glow surrounds both cores, suggesting a younger stellar population or ionized gas, hinting at a burst of star formation occurring throughout the system, but particularly in the areas around the center of the original galaxies. The overall morphology is disturbed, lacking a clear spiral or elliptical structure. Significant tidal features or extended arms are not readily apparent, suggesting that the merger may be in its early stages or that these features are too faint to be detected. The relative sizes of the two galactic nuclei appear similar, suggesting a merger between galaxies of comparable mass.
