The galaxy presents as a system with notable morphological disturbances, possibly indicative of an ongoing or recent interaction. There are three distinct clumps of luminous matter are observed, the brightest of which is yellow-white and the others are more red-orange. A compact object is located between these clumps of luminous matter, perhaps indicating the remnants of a nuclear core. The red-orange clumps are elongated in shape. The presence of these features suggests the galaxy is not a relaxed system and is likely undergoing a merger or strong tidal interaction with another galaxy.
