The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge that is bright and yellowish in color, suggesting a population of older stars. The outer regions of the galaxy fade gradually, with a less defined edge. There is a subtle hint of a disk-like structure, but it is not sharply defined, and the overall appearance is dominated by the smoothness and roundness of the elliptical morphology. There does not seem to be any obvious indication of strong spiral arm structure, bars, or major disturbances due to recent mergers. There may be very faint dust lanes or minor irregularities in the outer regions, but further observation is required to confirm this. The overall color suggests a galaxy that is primarily populated by older stars, with possibly limited ongoing star formation.
