The galaxy appears as a centrally concentrated object with a somewhat irregular, elliptical morphology. The core exhibits a bright, relatively uniform emission, suggestive of a dense stellar population or active galactic nucleus. A faint disk-like structure surrounds the central region, with hints of spiral arms. Faint tidal tails are evident extending from the main galactic body, which indicate gravitational interaction and a history of tidal interactions with companion galaxies. The galaxy exhibits a blue color in its central region, which may indicate the presence of younger stars. The edges of the galaxy exhibit a slight reddening, indicating an older stellar population. The overall structure suggests a galaxy that is likely undergoing a merging event.
