The galaxy exhibits a relatively smooth morphology with hints of a disk-like structure. It presents an elliptical shape, only slightly elongated. The central region is bright, potentially indicating a concentration of older stars or a possible active galactic nucleus. There are no signs of major disturbances or a recent merger event. Overall, the galaxy is a relatively well-formed system with a stable structure. There may be some degree of on-going star formation, but is likely happening at a slow rate.
