This galaxy exhibits a complex morphology indicative of a potential ongoing or recent merger event. The core of the galaxy displays a relatively smooth, concentrated structure, exhibiting a yellowish hue. The presence of an apparent tidal tail structure protruding from the main body suggests gravitational interaction with another galaxy. This could be the result of a smaller companion galaxy being tidally disrupted, or an advanced merger state. The light distribution is noticeably uneven, indicating an asymmetrical structure. There is a distinct blueish color present which shows areas of active star formation.
