The galaxy appears to be in a state of merging or strong interaction with another galaxy. The primary structure consists of what seems to be two distinct galactic nuclei or clumps of high stellar density. The brighter, lower component exhibits a greenish hue, possibly indicative of active star formation regions. The upper component presents a warmer, yellowish color. 

The overall shape is elongated with an estimated average radius of 1.2", deviating significantly from a perfect sphere. Tidal features or distortions appear present and would need further investigation. The galaxy exhibits a mixture of a smooth profile and visible features, potentially indicating a bulge component and disk-like structures affected by the ongoing interaction. There is likely a significant amount of dust and gas present within the system, given the color variations and irregularities observed.
