The galaxy presents an irregular morphology, indicative of an ongoing or recent interaction or merger event. Two distinct luminous regions are visible, suggesting either two separate galactic nuclei or regions of intense star formation triggered by a merger. The overall color appears moderately redder in one region versus the other, implying differences in stellar populations, dust content, or redshift. There are subtle wisps or tidal features extending from the main body of the galaxy, further supporting the interaction/merger hypothesis. The central region of the galaxy is relatively concentrated. Overall, the galaxy displays a complex and actively evolving structure.
