The galaxy appears to be undergoing a merger, exhibiting a disturbed morphology. Two distinct galactic nuclei are discernible; one more compact and brighter in the optical wavelengths, exhibiting a yellowish hue, and another less defined and somewhat fainter. The tidal interactions between the galaxies manifest as extended, diffuse arms or tails, stretching out from the main bodies.

A bluish tint is visible at the periphery of one of the interacting galaxies, potentially indicating areas of ongoing star formation. The overall color gradient suggests a complex stellar population, with both older, redder stars concentrated toward the center and younger, bluer stars in the outer regions. The system lacks a well-defined disk-like structure, consistent with the disruptive effects of an ongoing merger event. The relative proximity of the two galactic nuclei suggests this is an advanced stage merger.
