The galaxy presents a relatively smooth, elliptical morphology, though not perfectly spherical; it exhibits a slightly elongated shape. The core displays a pronounced concentration of light, with a yellow-orange hue indicative of an older stellar population. Moving outward from the central region, the color gradually shifts towards a bluer tone in the outer fringes, suggesting the presence of some younger, hotter stars, although the overall star formation rate appears to be subdued. There is no clear evidence of spiral arm structures or significant dust lanes. Minor disturbances may be present, though the galaxy appears mostly undisturbed without any signs of a recent major merger. 
