The galaxy presents an elliptical morphology, exhibiting a smooth, centrally concentrated light distribution. There is an absence of prominent spiral arms or a distinct disk structure. The color gradient transitions from a warmer, yellowish-orange hue towards the central region to slightly cooler tones in the outer areas, possibly indicating variations in stellar populations or dust content across the galaxy. There may be minor disturbances. The object is not particularly compact and likely represents a fairly massive system.
