The galaxy presents a disturbed morphology, characterized by an irregular shape suggestive of an ongoing or recent merger event. There's evidence of tidal features, possibly tails or bridges, indicating gravitational interaction with another galaxy. The central region displays a concentrated luminosity, potentially harboring an active galactic nucleus or a dense stellar population. The disk appears warped, and dust lanes are present but faint, hinting at obscuration and complex dynamics within the galaxy. Color variations suggest differing stellar populations and star formation activity in different regions, with bluer regions indicating ongoing star formation and redder regions indicating older stellar populations.
