This galaxy exhibits an elliptical morphology, appearing moderately elongated with a high degree of central concentration. The core region displays a bright, yellowish-white hue, indicating a likely older stellar population and potentially a supermassive black hole actively accreting material. A fainter, more diffuse halo surrounds the central region, gradually fading into the background sky. The color gradient suggests a radial distribution of stellar populations, with bluer stars potentially residing in the outer regions, although there are no discernable spiral arm structures or prominent star-forming regions visible. The smoothness of the light profile supports the classification as an elliptical galaxy, suggesting a history of mergers and dynamical relaxation. There are no obvious signs of tidal interactions or ongoing mergers, indicating the galaxy is likely isolated and relatively undisturbed.
