The galaxy presents as a smooth, elliptical structure, with a concentrated central bulge that radiates brightly in yellowish-orange hues. The overall form is not perfectly spherical, showing a slight elongation suggestive of an intermediate ellipticity. There are no immediately obvious spiral arm structures or dust lanes visible. Fainter, diffuse extensions are observable surrounding the central region, indicating a gradual decrease in stellar density towards the outer regions of the galaxy. There is no apparent major disturbance to the galaxy's structure suggesting a relaxed state. 
