The galaxy presents as a smooth, elliptical form with a high degree of central concentration. Its light profile is characterized by a relatively steep radial falloff, consistent with a high Sersic index. The color is generally reddish, becoming slightly bluer towards the outskirts. No prominent spiral arms or disk-like structures are discernible. The lack of obvious dust lanes or significant morphological disturbances suggests that the galaxy has not undergone a major merger event recently.
