The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a bright, concentrated central bulge, suggesting a high stellar density in its core. The overall color appears slightly reddish, indicating a population of older stars. A very faint blue halo is visible, meaning there is some new star formation. Based on the morphology, this galaxy likely has a substantial mass and potentially little ongoing star formation activity relative to its mass. There is no evidence of any major mergers. Minor disturbances may be present, however. The galaxy appears to be an intermediate shape between perfectly round and highly elongated.
