The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central region and a gradually decreasing intensity towards its edges. The core exhibits a yellowish-orange hue, suggesting an older stellar population and minimal ongoing star formation. The outer regions appear slightly redder than the core, possibly indicating the presence of older stars or dust. There are no visually prominent spiral arms or disk features. There are a few hints of very minor disturbances, but the galaxy appears largely undisturbed.
