The galaxy presents a complex morphology, suggesting an ongoing interaction or merger event. There are two discernible nuclei, one notably brighter and slightly more diffuse than the other. The brighter nucleus exhibits a yellowish-white hue, indicative of an older stellar population. A fainter, elongated structure extends downwards from this primary nucleus.

The second nucleus, positioned closer to the upper portion of the structure, appears more compact. There is a faint spiral arm structure radiating from the top nucleus, hinting at a disk-like component. A diffuse halo of light surrounds both nuclei, connecting them in a single, unified system. This envelope exhibits a mottled texture, possibly due to dust lanes or tidal debris.

The overall color gradient suggests a mix of stellar populations, with older, redder stars concentrated within the central bulge region. Some distortion is observed within the shape of the galaxy, a possible sign of recent tidal forces.
