The galaxy appears to be a merger in progress, exhibiting a disturbed morphology. Two distinct, bright cores are visible, suggesting two separate galactic nuclei. The overall color is yellowish, indicating an older stellar population. There is faint, extended material surrounding the central cores, likely tidal debris from the interaction. No prominent spiral arms or dust lanes are discernible; the structure seems largely amorphous. The smooth light profile overall seems to indicate that it is primarily composed of older stars.
