This galaxy appears to be undergoing a merger, with a significant amount of tidal disturbance visible. The system exhibits a complex morphology, showing characteristics of both a smooth, elliptical-like structure, and more defined, disk-like features. One component displays a relatively round profile, while the other is more elongated. There is evidence of ongoing star formation, particularly within the disturbed regions, indicated by bluer colors. A significant portion of the light is concentrated in the central region, suggesting a relatively high density of stars. The color gradient is relatively smooth, with a gradual shift from bluer to redder hues towards the galaxy's core.
