The galaxy appears as a smooth, elongated structure, possibly a lenticular or elliptical galaxy viewed at an oblique angle. Its central region exhibits a concentrated, yellowish-white luminosity, suggesting an older stellar population. The outer regions display a gradual decrease in surface brightness, fading into the background. There may be some minor disturbances visible within the galaxy. The overall color index suggests a relatively evolved system with lower rates of recent star formation. The galaxy is moderately large and exhibits significant luminosity.
