The galaxy presents as a merging system, characterized by two distinct luminous components. The primary component exhibits a smooth, elliptical morphology. Its color is predominantly yellow, suggesting an older stellar population. There is a minor disturbance near the primary component suggesting an interaction or merging event. 

The secondary component, positioned below the primary, is less defined. This component displays a bluer hue along the lower edge, hinting at possible ongoing star formation within a disk-like structure. The overall light distribution in the galaxy is smooth. A larger system could be formed through this interaction with limited star formation.
