The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a high surface brightness, with the intensity gradually decreasing towards the outer edges. The overall shape is somewhat elongated, with the major axis extending in a northwest-southeast direction. There is a subtle hint of a disk-like structure, but it is not sharply defined. No distinct spiral arms are discernible. Color gradients suggest a population of older stars dominating the galaxy's stellar content. The galaxy appears relatively undisturbed, without evidence of significant tidal interactions or major merging events.