The galaxy exhibits a disturbed morphology, potentially indicative of a merger event. Two distinct, brighter cores are visible, suggesting either two galactic nuclei in close proximity or a single nucleus with significant tidal disruption. Faint, diffuse material connects these cores, appearing as a bridge or tail-like structure. There appears to be blueish star formation regions towards the outer regions of the galaxy. The overall color of the central region is reddish, indicative of older stellar populations or dust obscuration. Given the extent of the disturbance, a significant fraction of the galaxy's mass is likely involved in this interaction, making it a relatively massive system. Star formation appears to be actively taking place, although the rate may not be exceedingly high, based on the limited extent of the blue regions. The galaxy's overall appearance is complex and dynamically active, characteristic of interacting or recently merged systems.
