This galaxy exhibits an overall elliptical morphology, appearing largely smooth and centrally concentrated. The light distribution suggests a dominant bulge component, characterized by a gradual decrease in surface brightness from the core outwards. There's a notable absence of prominent spiral arms or distinct features indicative of active star formation, as evidenced by a lack of strong blue color gradients. The galaxy's color profile suggests a population of older stars. There are no clear signs of ongoing mergers or major tidal disturbances, and appears relatively undisturbed.
