The galaxy presents a reddish-yellow hue, suggesting a relatively older stellar population. Its morphology appears to be that of a disk galaxy with an apparent size of around 8.5 kpc. The galaxy's smoothness suggests it is likely elliptical or an early-type spiral. However, the image suggests some merging of another galaxy. The galaxy shows signs of interaction with another galaxy. The relative absence of blue light implies a low star formation rate.
