The galaxy appears as a somewhat elliptical, smooth object. It exhibits a concentrated central bulge that is bright and slightly bluish in color, suggesting a population of younger stars. The surrounding halo appears redder, possibly indicating an older stellar population. There is no visible dust lane or spiral arm structure discernible within the image. Overall, the galaxy seems relatively undisturbed, lacking any obvious signs of a recent major merger event, though there may be very minor disturbances. The galaxy is moderately large, appearing to be a massive galaxy with a notable halo structure.
