The galaxy presents as a generally smooth, though somewhat disturbed, object. It appears to be undergoing a significant merger event. The primary body of the galaxy exhibits a yellowish hue, suggestive of an older stellar population. Two distinct nuclei are visible within the galaxy, indicating two previously separate galactic centers in the process of coalescing. A faint blueish tinge surrounds the yellowish core, suggesting ongoing, albeit potentially low-level, star formation activity. The galaxy exhibits a moderate degree of roundness, with only minor tidal disturbances visibly emanating from the interaction. Overall, the galaxy appears to be a luminous, merging system with evidence of past or ongoing star formation.
