The galaxy presents as a largely smooth, centrally concentrated object. The light profile appears elliptical with some deviation from a perfect ellipse. The central region is bright and yellowish, suggesting an older stellar population. The outer regions are fainter and redder in color, indicating either a difference in stellar population or dust extinction. There is no apparent spiral structure or bar, and no evidence of any ongoing major merger events. There is a subtle disturbance on the outer halo of the galaxy, and there is a slight disk-like structure.
