The galaxy presents a relatively smooth and concentrated morphology. Its overall shape appears elliptical, displaying an approximate circular symmetry. The galaxy's color profile suggests a dominant older stellar population, with a yellowish-orange hue across its body, which points to stars that are in the later stages of their life cycle. There is a lack of noticeable spiral arm structures or dust lanes in the image. The galaxy's light is brightest at the center, with a gradual decrease in luminosity toward its outer edges. There is no clear evidence of any major ongoing merger events, though minor disturbances might be present.
