This galaxy exhibits a morphology suggesting a system undergoing significant interaction or merging. The core region presents a bright, concentrated luminosity, possibly indicative of a dense stellar population or active galactic nucleus. Faint, diffuse tidal features emanate from the central body, extending in multiple directions. These plumes suggest gravitational disruption and mass transfer between interacting components. The overall structure appears irregular, lacking a well-defined spiral or elliptical form. There is evidence of potential dust lanes or obscuring material within the galaxy, appearing as subtle color variations in the diffuse regions. The general color of the galaxy leans towards a bluer hue in the outer regions, suggestive of ongoing star formation, although redder, more evolved stellar populations may be present in the central bulge and tidal features. Overall, the galaxy appears to be in a state of dynamic evolution resulting from a major disturbance.
