This galaxy appears to be in a late-stage merger or experiencing significant tidal disruption. The central region exhibits a bright, somewhat diffuse core with two possible nuclei, indicating the remnants of two merging galaxies. A prominent tidal tail extends outwards from the main body, curving away into the surrounding field. This tail has a bluer color than the central region, implying the presence of younger stars formed as a result of the interaction. The overall color suggests an older stellar population, with a mix of evolved stars and possibly some ongoing star formation concentrated in the tidal tail. There are other features near the core that could either be the remnants of tidal features or areas of increased star formation activity. The galaxy is not perfectly symmetrical, reinforcing the disturbance from a recent or ongoing merger event.
