The galaxy presents as a relatively smooth and centrally concentrated object. Its overall morphology appears to be elliptical, with a slight elongation. The color profile suggests a dominance of older stellar populations, with a yellow-red hue characterizing the galaxy's core and a gradual fading toward the outer regions. There is little evidence of spiral arm structures or significant dust lanes from what can be visually gathered in the image, reinforcing the classification of it as a smooth galaxy. No signs of any current major or minor merger events are visible.
