This galaxy exhibits an elliptical morphology, appearing as a smooth, elongated spheroid. The central region displays a concentrated luminosity, indicative of a dense stellar population, likely dominated by older stars. The light profile transitions smoothly from the bright core outwards, diminishing in intensity towards the edges, with no distinct spiral arm structures visible. The color profile suggests a higher concentration of older, redder stars within the central bulge, transitioning to slightly bluer hues in the outer regions. Overall, the galaxy's structure indicates a relatively evolved system with a high degree of internal order. No signs of any recent major merger event are readily apparent.
