The galaxy appears as a roughly circular, concentrated luminous object. The core exhibits a yellowish-white hue, suggesting a population of older stars. A subtle greenish-blue halo surrounds the core, possibly indicating some ongoing, albeit low, star formation. This outer region is less defined and fainter than the central core. The galaxy's overall structure seems largely smooth, with no apparent spiral arms or significant disturbances, suggesting it is likely an elliptical galaxy. There is a hint of asymmetry on one side, although this could be the result of image artifact. No signs of a major ongoing merger are evident, although a minor interaction cannot be ruled out.
