The galaxy appears to be a relatively smooth, elliptical system. It exhibits a centrally concentrated luminosity profile with a distinct yellowish hue, suggesting an older stellar population. Its round shape indicates a classification of E0-E3 on the Hubble sequence. There might be some minor tidal disturbances or asymmetries in the outer halo, but the overall structure is largely undisturbed. Although the image doesn't resolve individual stars, the color suggests a lack of recent star formation activity. There is a possibility of a close interaction or merger in the past given the minor disturbances. Overall, it resembles a massive, quiescent elliptical galaxy at a considerable distance, characterized by a high degree of sphericity and evolved stellar content.
