The object is a single galaxy exhibiting signs of a major merger or significant interaction with another galaxy or galaxies. The light distribution is complex and irregular. There is a large central, yellowish-orange component. This central region may indicate the presence of older stars. The overall shape is irregular, lacking any defined spiral structure or elliptical form. The system's size suggests it's a relatively large galaxy. The apparent magnitudes and inferred absolute magnitudes suggest this is a luminous object. There may be a secondary bright, relatively round component to the right of the main body, which could either be a component of the on-going merger or a background object, but its proximity and alignment suggest it may be an integral part of this system. Overall, the galaxy shows strong indications of a dynamic, potentially disruptive event in its recent past or present.
