The galaxy exhibits a complex morphology, suggestive of an ongoing or recent merger event. Two distinct luminous components are discernible. The brighter, lower component displays a yellowish-orange hue, potentially indicating an older stellar population. Its shape is elongated and irregular, deviating from a spheroidal morphology.

The upper component appears less luminous and exhibits a more greenish-yellow color, possibly indicating a younger stellar population or increased star formation activity. This component also exhibits a non-spherical shape. 

A bridge-like structure or tidal feature appears to connect these two components, indicating gravitational interaction. Faint, diffuse light surrounds the merging system. The presence of significant disturbances in the overall morphology supports the hypothesis of a major merger. The system is compact.
