The galaxy exhibits a disturbed morphology, suggestive of an ongoing or recent interaction. Two distinct luminosity concentrations are apparent, potentially representing the cores of merging galaxies. One concentration appears more diffuse with a bluer hue, possibly indicating active star formation regions. The second, brighter concentration shows a redder color, which could indicate an older stellar population. A faint tidal tail-like structure can be discerned, further supporting the interpretation of a merging system. Overall, the galaxy presents as a complex system in a dynamically active phase.
