The galaxy presents a predominantly smooth morphology, with a subtle, extended halo of diffuse light surrounding a bright, concentrated central region. The color gradient suggests a moderate amount of star formation, indicated by a slightly bluer hue within the central regions compared to the outer halo, where older stellar populations likely dominate, imparting a redder tone. There may be a hint of a disk structure, but the smoothness suggests it is either viewed close to face-on or is a more spheroidally dominated system. There is no obvious sign of any merger activity or major disturbances affecting its overall structure. The galaxy is generally round in appearance, although there is some deviation from perfect circularity.
