The galaxy presents a largely smooth, elliptical morphology. Its color gradient suggests a concentration of older stellar populations, appearing yellow in the core, with subtle bluer regions present in the outer halo. The light is highly concentrated toward the center. There is no prominent disk or spiral arm structure observed within this image, nor is there any obvious evidence of a major merger event, tidal tails, or strong gravitational disturbances affecting its overall structure. There are no apparent dust lanes or strong star forming regions either. The galaxy is classified as a relatively round, non-disturbed system.
