The galaxy appears as a moderately bright, elliptical-shaped object. Its core exhibits a high degree of luminosity, suggesting a concentration of older stellar populations and possibly a supermassive black hole at the center. Moving outwards from the core, the luminosity gradually diminishes. The overall color appears relatively uniform, trending towards the redder end of the spectrum. There is a subtle hint of a disk-like structure, but the galaxy is dominated by its elliptical morphology. No strong indications of active star formation are visually apparent, nor are any signs of ongoing major mergers or significant tidal disturbances. The galaxy presents as a relatively smooth, undisturbed system.
