The galaxy appears to be elliptical in shape, although not perfectly circular. Its central region exhibits a concentrated, bright core which gradually diffuses outwards. The color profile suggests an older stellar population, with a yellowish-white hue dominating the central region. The outer regions display a bluer tint, hinting at the presence of younger stars or a different stellar population mix, but this is less pronounced. There is no obvious spiral arm structure or dust lanes visible. The galaxy presents a smooth, relatively featureless morphology. It appears undisturbed, showing no strong signs of recent mergers or interactions, and has an apparent orientation that is slightly tilted.
