The galaxy exhibits a primarily smooth morphology, with an overall elliptical shape. The core region presents a bright, concentrated luminosity, suggesting a high stellar density. Moving outwards from the core, the light intensity gradually diminishes, transitioning into a more diffuse halo. The galaxy appears mostly undisturbed, with minimal evidence of significant tidal interactions or mergers. A subtle color gradient can be observed, with the central region exhibiting a yellow/orange hue, potentially indicative of an older stellar population, while the outer regions show a slight bluish tint, which might suggest more recent star formation.
