The galaxy presents as a centrally concentrated elliptical system. The core exhibits a bright, yellowish-white hue, suggesting an older stellar population. A smooth, diffuse halo extends outward, fading in intensity. There are some subtle blue tinges in the halo, suggesting the possibility of some younger star formation. The galaxy shows a high degree of symmetry and roundness, lacking any obvious spiral arm structures or significant morphological distortions suggestive of ongoing or recent major mergers. The galaxy appears relatively isolated in this image, showing no close companions that could be influencing its structure.
