This galaxy exhibits a disturbed morphology, likely indicative of an ongoing or recent merger event. A distinct tidal tail is visible, extending outwards from the main galactic body. The central region presents a bright, concentrated area of older stars. A significant portion of the galaxy appears to be actively forming stars, as evidenced by the bluer regions, most notably present towards the outer edges and the tidal feature. Overall, the galaxy demonstrates significant signs of dynamical interaction.
