The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that gradually diffuses into the outer regions. The galaxy's color is predominantly yellow-orange, which suggests an older stellar population. The overall shape is fairly rounded. There is no discernible spiral arm structure or any evidence of ongoing major merger activity. Minor disturbances cannot be ruled out, though the galaxy appears relatively undisturbed. The color distribution is rather uniform, showing minimal signs of active star formation regions. The galaxy is likely a massive system.
