Observed is a system exhibiting a central, elliptical galaxy and what appears to be a spiral galaxy engaged in a gravitational interaction. The elliptical galaxy presents a smooth, relatively featureless profile, dominated by older stellar populations, indicated by its yellow-orange hue. The spiral galaxy displays a defined spiral arm structure, though somewhat disturbed, with regions of likely ongoing star formation marked by a bluer color. Indications show that the two are undergoing a significant merger event. There appears to be a tidal tail or bridge of material emanating from the spiral, further suggesting a disruptive interaction with the elliptical component. There are regions of increased intensity in the spiral disk indicative of star formation. Overall, the system appears to be dynamically active, with evidence of significant morphological disturbance.
