The galaxy presents as a relatively smooth, elliptical-shaped object with a concentrated central bulge. It appears to be a mature system, exhibiting a yellowish-orange hue that suggests an older stellar population with a relatively low rate of ongoing star formation. The galaxy shows a slight elongation, and subtle hints of a disk-like structure may be present but not sharply defined. There are no prominent spiral arms or active star-forming regions visible. The light distribution smoothly decreases from the bright center, indicating a lack of significant dust lanes or other obscuring material. The overall color suggests it is a massive galaxy. There is no obvious evidence of a recent major merger or tidal disturbance.
