The galaxy presents as a largely smooth, centrally concentrated structure. It exhibits an elliptical morphology, with a high degree of radial symmetry. The core region displays a bright, yellowish-white luminosity, indicative of a concentrated population of older stars. Moving outward from the center, the light gradually diminishes, showing a subtle color gradient towards redder hues in the outer regions. There are no apparent spiral arms or distinct dust lanes visible within the galaxy's structure. A slight deviation from perfect ellipticity hints at a possible minor interaction or internal disturbance, but it is largely unpronounced. Overall, the galaxy appears to be a relatively quiescent, evolved system.
