The galaxy presents as an elliptical structure, with a high degree of central concentration. The core region exhibits a significantly brighter luminosity than the surrounding halo. The overall color appears yellowish, suggestive of an older stellar population dominating the galaxy's composition. There is little evidence of distinct spiral arms or significant dust lanes. The galaxy's shape deviates slightly from perfect circularity, exhibiting a mild elongation. No obvious signs of recent mergers or tidal disturbances are immediately apparent. The galaxy appears relatively smooth in texture with its light distribution, hinting at a well-mixed stellar population.
