This galaxy appears to be undergoing a significant interaction or merger. The system displays a disturbed morphology, characterized by multiple luminous components. A primary, somewhat diffuse component exhibits a yellowish hue, possibly indicative of an older stellar population. A fainter, elongated structure extends from this primary component, displaying a reddish color, suggesting dust obscuration or a population of redder stars. A bluer, more compact object is also apparent and separate from the other objects. The presence of these distinct components and irregular shapes suggests that this is not a relaxed system and may even be in the final stages of a galactic merger. The overall system exhibits relatively high luminosity, implying substantial stellar mass and ongoing star formation activity.
