The galaxy presents a largely smooth, featureless appearance. It appears predominantly round in shape. The galaxy's core exhibits a more intense concentration of light, which gradually diminishes towards its outer regions. Color analysis indicates a concentration of older stellar populations, particularly within the galaxy's central bulge. This is supported by the high red color index. There is some evidence of minor irregularities or disturbances in the outer regions, possibly indicating past or ongoing interactions with smaller galaxies.
