The galaxy appears to be an interacting system composed of two distinct galactic nuclei or clumps of high stellar density. The overall morphology suggests a merger in progress. Both cores display a yellowish hue, indicating an older stellar population within. A reddish concentration is visible between them, possibly denoting an area of active star formation triggered by the gravitational interaction. Diffuse, faint material surrounds the central components, hinting at tidal tails or distorted galactic arms due to the ongoing merger event. The system's overall shape deviates significantly from a regular elliptical or spiral morphology.
