The galaxy appears to be an interacting system, potentially undergoing a merger. There are at least two distinct nuclei visible, one slightly more diffuse and elongated than the other. Both display a yellowish hue suggestive of an older stellar population, although some bluer regions hint at ongoing or recent star formation. There's an indication of tidal features, or disturbances, extending from the main bodies of the galaxy, further supporting the ongoing merger hypothesis. The overall morphology appears complex and irregular.
