This galaxy presents a largely smooth, elliptical morphology. The core exhibits a strong, concentrated luminosity gradient, appearing intensely bright. Moving outward from the core, the luminosity decreases gradually with no distinct breaks or structures. The overall color appears somewhat redder, likely indicating an older stellar population and diminished current star formation activity. There are no obvious spiral arms or a central bar structure discernible in the image, suggesting that it is not a spiral galaxy. Minor disturbances cannot be ruled out. 