The galaxy presents as a moderately bright, elliptical form. The central bulge appears significantly brighter and more concentrated than the outer regions, indicating a substantial stellar population. There is a noticeable color gradient, with the core exhibiting a yellowish-orange hue, possibly indicative of older stellar populations and/or dust obscuration. The outer regions appear slightly bluer, potentially due to younger stars. The galaxy appears largely undisturbed with a smooth morphology, with a slight hint of a disk structure viewed nearly edge-on. There is no strong evidence of ongoing major mergers or significant tidal distortions.
