The galaxy presents as a single, relatively smooth, concentrated light source. It appears to be elliptical in shape, displaying a high degree of circularity. There is a distinct color gradient, with the central region exhibiting a strong yellow-orange hue, suggesting an older stellar population dominated by redder stars. The outer regions of the galaxy show a gradual decrease in luminosity and a subtle shift towards a slightly bluer tone, potentially indicating the presence of younger stars, although this feature is not very prominent. There is no apparent spiral structure, bar, or signs of active galactic nuclei. There does not appear to be any merger activity or interaction with other galaxies occurring in the image. Overall, this galaxy seems to be a passively evolving system with a substantial population of older stars.
