This galaxy exhibits characteristics suggesting an ongoing or recent merger event. The system appears to comprise two distinct components. The primary component presents a diffuse, somewhat irregular morphology, exhibiting a dominant bluish hue indicating the presence of a substantial population of young, hot stars, likely indicative of recent star formation. This component's shape is somewhat elongated. The secondary component is smaller and displays a more concentrated, yellowish color, suggesting an older stellar population, potentially the core of another galaxy or a dense galactic nucleus. This secondary component exhibits a more spheroidal appearance. There is evidence of tidal features or disturbed morphology, particularly between the two components, further supporting the hypothesis of an interaction or merger. The overall luminosity of the system is relatively high. Based on its redshift, this galaxy is at a considerable distance.
