The galaxy appears to be in a late-stage merger, exhibiting significant morphological disturbance. Two distinct nuclei are visible: a brighter, bluer nucleus located toward the lower portion of the image and a dimmer, yellower nucleus positioned above it. Diffuse tidal features are present, enveloping both nuclei, suggesting gravitational interaction and stellar disruption. The overall color gradient across the galaxy indicates variations in stellar populations, with the bluer regions likely indicating areas of recent star formation. The galaxy's shape is highly irregular, lacking any clear spiral arm structure or elliptical symmetry. There may be a possible minor secondary structure in the tidal tails. 
