The galaxy exhibits a disturbed morphology, suggestive of an ongoing or recent interaction or merger event. It presents an elongated shape, appearing somewhat cigar-shaped. The light distribution indicates at least two distinct bright regions, one of which is yellower in color and the other is more reddish-orange. A region of bluer emission is also apparent near the center. The system displays an overall smooth profile with the central region appearing more diffuse compared to the brighter regions. It appears to be an interacting system with an estimated mass of 10^10 Msun. The light from this galaxy has been redshifted approximately 24%, indicating its considerable distance from our own. The color properties suggest some ongoing star formation is likely present, though not dominating the emission.
