The galaxy appears to be a merging system, possibly in the late stages of interaction. Two distinct, roughly spherical components are visible, each exhibiting a yellowish-orange hue suggestive of an older stellar population with minimal ongoing star formation. The morphology of each component is smooth, lacking significant disk-like features or spiral arm structures. There is a possible tidal tail or bridge of material extending between the two components, although this is uncertain due to the image quality. The overall appearance suggests a relatively massive system with a redshift corresponding to a significant distance, indicating that we are observing the galaxy as it was billions of years ago. There appears to be evidence of minor disturbances to the galaxy's structure.
