This galaxy exhibits a morphology indicative of a significant interaction or merger event. The primary body displays a relatively smooth, ellipsoidal appearance, suggesting an evolved stellar population. However, a distinct tidal tail extends from the galaxy, characterized by a reddish hue, potentially indicating ongoing or recent star formation within the stripped material. The main galactic body presents a yellow-orange color gradient, which could be attributed to a mix of older stellar populations and dust obscuration. There also appears to be a secondary concentration of luminosity offset from the main body, suggesting either a partially merged companion galaxy or a region of intense star formation triggered by the interaction. Overall, the galaxy appears to be a system in a dynamic state, undergoing significant morphological transformation due to gravitational interactions.
