The galaxy appears to be undergoing a major merger event. The primary body exhibits a somewhat amorphous morphology, displaying a central concentration of light, likely indicative of an older stellar population. Diffuse, extended arms or tidal tails extend from the main body, demonstrating clear signs of gravitational interaction and disruption. There's an additional component beside it, in a roughly elliptical shape, appearing brighter, perhaps a secondary galaxy undergoing the process of merging with the primary. The overall color profile suggests a mix of stellar populations; with the central region exhibiting a warmer hue, indicative of older stars or dust obscuration, while the outer regions show a cooler, bluer coloration. Evidence of ongoing star formation may exist within the tidal features.
