The galaxy presents as a centrally concentrated, elliptical-like structure. It exhibits a relatively smooth light distribution, with a high degree of radial symmetry. The central region is bright and appears yellowish-white, suggesting a population of older stars. There is a subtle color gradient, with the outer regions appearing slightly redder than the core. No distinct spiral arm structures or significant dust lanes are discernible, reinforcing the impression of a relatively quiescent, early-type galaxy. Minor disturbances and a faint red streak are visible at the periphery, hinting at a possible minor interaction or past merger event. Overall, the galaxy's morphology points toward a relatively evolved system.
