The galaxy presents as a merging system. The structure is complex, appearing as two distinct luminous regions in close proximity. One region exhibits a more diffuse, smooth characteristic, while the second appears slightly more compact and defined. A faint bridge of material seems to connect the two galactic nuclei, suggesting a tidal interaction. Overall, the system displays a yellow/white hue. We see no clear spiral arm structure or well-defined dust lanes. The disturbed morphology suggests the system is currently undergoing a significant interaction that has altered its overall shape and distribution of stellar material.
