This galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a centrally concentrated luminosity profile, with the brightest region located at the core. The overall shape is generally round. There is no visually apparent evidence of spiral arms, a disk structure, or any significant tidal disturbances suggesting recent major merger events. The galaxy has a redder hue, especially in the outer regions, which suggests an older stellar population with diminished ongoing star formation.
