The galaxy presents as a largely smooth, elliptical-like structure. The core exhibits a concentrated, yellowish-white luminosity, suggesting a substantial population of older stars. Surrounding the core, a fainter, diffuse halo extends outward, displaying a subtle gradient of decreasing brightness. Hints of a slightly bluer hue in the outer regions may indicate some ongoing star formation. There are no obvious spiral arms or a distinct disk component visible in the image. The galaxy appears relatively undisturbed, without significant signs of recent mergers or tidal interactions, although a very slight asymmetry could suggest minor gravitational disturbance. The overall morphology points toward a massive galaxy with a relatively low star formation rate.
