The galaxy presents as a slightly elongated, elliptical structure with a smooth, diffuse appearance. The core region is relatively bright and concentrated, exhibiting a yellowish-orange hue, indicative of an older stellar population. There is a subtle falloff in luminosity from the core outwards, lacking any distinct spiral arm features or prominent dust lanes. The outer regions appear fainter and more diffuse, blending gradually with the background sky. No obvious signs of recent merger activity or significant morphological disturbances are apparent. The galaxy appears relatively isolated and undisturbed.
