The galaxy presents a generally smooth, elliptical morphology. There is a concentrated central bulge with a gradual fading of luminosity towards the outer edges. The galaxy's shape is more rounded. Evidence suggests a possible ongoing or recent major merger, indicated by some disturbed features in the outer halo of the galaxy. The color appears to be reddish, suggesting an older stellar population with lower ongoing star formation. The apparent size suggests a massive galaxy. Overall, the galaxy seems to be a passively evolving elliptical with signs of a past or current interaction.
