This galaxy exhibits a morphology indicative of an ongoing or recent merger event. The overall structure is complex, with what appears to be two distinct, bright nuclei, possibly the cores of the original merging galaxies. The dominant color of the galaxy is redder, suggesting an older stellar population, with an apparent lack of significant ongoing star formation activity. There is also a notable extended tidal tail extending downwards. The galaxy's shape is generally elliptical, but the disturbances indicate that it is not entirely uniform or relaxed in morphology. A few irregularities or faint regions that could indicate residual star formation pockets can be seen. There is some overall asymmetry, reinforcing the impression of dynamical disturbance.
