The galaxy presents as a single, relatively compact object with a smooth, elliptical morphology. There are no visually apparent spiral arms or a distinct disk structure. The galaxy displays a color gradient, appearing more yellow and orange towards its core, suggesting a population of older, redder stars concentrated centrally. The outer regions exhibit a bluer hue, potentially indicating a younger stellar population or ongoing, though subdued, star formation activity. There is a slight asymmetry in the outer halo, which may be due to a minor gravitational interaction or disturbance. Overall, the galaxy appears to be a massive, evolved system with signs of minimal ongoing star formation.
