The object appears to be a galaxy at a significant distance, exhibiting a redshift. The galaxy has a generally smooth appearance, but with some visible features suggesting internal structure or possible interactions. The shape can be characterized as somewhere between round and elongated, leaning toward an intermediate form. The galaxy's color profile indicates that there may be ongoing or recent star formation. The galaxy does not seem to be isolated, appearing to undergo a possible merger with another galaxy. There is some visual evidence suggesting minor disturbances. The light distribution within the galaxy is not entirely uniform, showing some clumping or asymmetries that may contribute to the ongoing merger event.
