The galaxy appears to be in the late stages of a merger, presenting as two distinct, luminous cores embedded within a common, fainter halo. The two cores are separated by a relatively small distance and exhibit a yellowish-white hue, potentially indicative of an older stellar population. Faint tidal tails and bridges of material connect and extend outward, suggesting significant gravitational interaction. There is a slightly extended shape to the overall structure. The halo has some regions of blue/green that could indicate star formation. The galaxy system appears dynamically disturbed, lacking a clear, well-defined spiral or elliptical structure. 
