The galaxy presents as a relatively smooth, elliptical object. It exhibits a concentration of light towards the central region, with a gradual decrease in brightness towards the outer edges. The color profile appears yellowish-white, suggesting a population of older stars. There is a hint of a subtle disk-like structure although, overall, the morphology is smooth and featureless. No distinct spiral arms or prominent dust lanes are discernible. There are no signs of major interaction or merging events; the galaxy appears relatively isolated.
