This galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a centrally concentrated luminosity profile, with a bright, yellowish core that gradually fades into the surrounding galactic halo. There is minimal evidence of spiral arm structures or significant dust lanes. The overall shape appears somewhat rounded, with a slight deviation from perfect circularity. Indications are that the system appears relatively undisturbed, showing little sign of on-going major merging events or tidal disruptions. There is a faint hint of bluer hues in the outer regions, suggesting the presence of some younger stars. However, the dominant color throughout the galaxy is indicative of an older stellar population. The galaxy exhibits a moderate redshift, indicating that it is at a considerable distance from us. The image suggests the galaxy possesses a substantial mass.
