This galaxy exhibits a disturbed morphology suggestive of a merger event. The central region displays a bright, concentrated core, possibly indicative of an active galactic nucleus or a dense concentration of stars. Extending outward from the core, there are faint, diffuse structures with irregular shapes. A noticeable arm-like feature appears to extend from the core, displaying a bluish hue possibly indicating the presence of younger stars. There appears to be a slight degree of asymmetry in the galaxy's overall structure, supporting the presence of an ongoing or recent merger.
