The galaxy appears as a roughly circular object, though its morphology is somewhat disturbed or irregular. There is a bright, concentrated central region, possibly a bulge or active galactic nucleus, exhibiting a green/yellow hue. The surrounding region presents a more diffuse, blue-ish distribution of light, potentially indicative of younger stellar populations or ongoing star formation. There are indications of some arm-like structure or features extending outward from the central region, but these are not well-defined and suggest a disrupted or irregular morphology, possibly due to gravitational interactions. There seems to be some tidal debris or a faint tail extending on opposing sides of the galaxy. The general color profile suggests a galaxy with a mix of stellar ages, with a relatively older population concentrated in the center and younger, bluer stars distributed in the outer regions and arms. Based on the appearance, the galaxy is likely undergoing some form of interaction or merger activity, leading to its distorted structure.
