The galaxy presents a largely smooth, elliptical morphology. Its central region is a bright, concentrated bulge that appears almost spherical in shape. Moving outwards from the center, the light gradually diminishes, with a more diffuse halo surrounding the central bulge. There's little evidence of spiral arm structures or prominent dust lanes within the resolution limits of this image. The color profile shows a concentration of yellow light in the core, hinting at an older stellar population dominating this region. The outer edges show hints of bluer hues, which could be an indicator of some ongoing, albeit weak, star formation activity. Overall, the galaxy appears relatively undisturbed and isolated, with no obvious signs of major mergers or tidal interactions. The light distribution appears quite symmetric, furthering the assessment of a relaxed and evolved system.
