The galaxy exhibits an apparent morphology indicative of an ongoing or recent merger event. Two distinct nuclei are visible within a common, diffuse halo. One nucleus appears brighter and more compact than the other, exhibiting a yellowish hue. The second nucleus is slightly less defined, with a less concentrated light profile. There is some evidence of tidal distortion or extended features emanating from the merging components, but they are faint. Overall, the galaxy appears relatively smooth and featureless, though the merger process disrupts any clear spiral or elliptical structure. Its red shift implies that the light we are seeing has shifted significantly to the red end of the spectrum, indicating that the galaxy is receding from us. The galaxy is moderately luminous, and has an estimated mass within a specific range. The galaxy exhibits evidence of moderate star formation.
