The galaxy appears to be undergoing a possible merging event or displaying some form of significant interaction. The central region exhibits a bright, somewhat amorphous structure, with a dominant cyan hue. This suggests active star formation or an Active Galactic Nucleus (AGN). The light distribution is not uniform, showing indications of internal structures or clumps. The overall shape deviates significantly from a regular elliptical or spiral, indicating a disturbed morphology. There is a possible tidal tail or stream-like feature extending from one side of the galaxy. This feature has a reddish color, and it could be indicative of older stellar populations. The galaxy shows indications of ongoing or recent interaction with another galaxy or internal instability. There is a faint yellow area in the disk, which would indicate slightly older stars.
