The galaxy presents as an elliptical morphology, exhibiting a generally smooth appearance with no readily discernible spiral arm structures or dust lanes. It has a moderate degree of ellipticity, appearing somewhat elongated rather than perfectly spherical. The central region of the galaxy is characterized by a bright, concentrated core, suggesting a high stellar density. Moving outward from the core, the luminosity gradually decreases, displaying a diffuse halo that blends into the background sky. The galaxy exhibits a color gradient, with the core appearing yellower and the outer regions appearing slightly bluer. Overall, the galaxy seems relatively undisturbed, showing no obvious signs of recent mergers or tidal interactions.
