The galaxy appears to be undergoing a significant merger. Evident are two distinct galactic nuclei, one displaying a yellowish-orange hue, indicative of an older stellar population, and the other a bluer tint suggesting recent star formation. There are signs of major gravitational disturbance. The primary body displays an irregular morphology, lacking a well-defined spiral or elliptical structure. The overall shape is amorphous, indicating strong tidal forces are at work. The separation between the nuclei is relatively small. There are faint wisps of material extending outwards, possibly tidal tails formed during the interaction. The galaxy exhibits a moderate luminosity. The galaxy is likely at a considerable distance, given the observed redshift, and the inferred size suggests it is a moderately sized galaxy. There appears to be minimal ongoing star formation.
