The galaxy presents as a well-defined elliptical structure, elongated along its major axis. The central region exhibits a high surface brightness, with a yellowish-white color indicative of an older stellar population. Surrounding this core is a more diffuse halo, showing a pinkish hue. This suggests the presence of a small amount of ongoing star formation, possibly due to gas accretion or a minor merger event in the relatively recent past, but otherwise the lack of intense blue color indicates that the galaxy is mostly composed of older stars. The overall smoothness of the galaxy suggests a relatively relaxed system, with minimal signs of major recent disturbances or mergers. The morphology is consistent with an evolved galaxy that is in the process of slowly quenching its star formation activity.