The galaxy presents a largely smooth, elliptical morphology. The light profile appears centrally concentrated with a radial falloff in intensity. The core exhibits a yellowish-orange hue, suggesting an older stellar population. There is little evidence of spiral arm structure or significant dust lanes within the visible portion of the galaxy. The overall shape is close to round, with a slight deviation toward an intermediate elliptical form. No obvious signs of recent or ongoing major mergers are apparent, though there may be a minor asymmetry to the outskirts of the object. There may be some evidence of blue light in the galaxy's extremities, suggesting some younger star formation.
