The galaxy appears to be undergoing a merging event, with two distinct, luminous regions present. One region appears more rounded in shape, while the other is slightly more elongated or diffuse. There is evidence of tidal disturbances or distortions in the overall structure, though the merging process does not seem to involve a major disruption of either galaxy. The galaxy displays a smooth, featureless morphology, indicating a lack of prominent spiral arms or well-defined dust lanes. The color is consistent with an older stellar population. Overall, this appears to be a relatively massive system with a moderate rate of star formation, viewed at a redshift indicative of significant cosmological distance. The galaxy exhibits intermediate roundness between circular and cigar-shaped.