The galaxy presents as a single, relatively symmetrical, concentrated mass of stars. It is elliptical in shape, displaying a smooth morphology with a high degree of central concentration that is quite round. Its core exhibits a yellowish hue, which gradually fades into a more diffuse, reddish halo. There are no visually discernible spiral arms, bar structures, or obvious signs of recent or ongoing major merger activity. Faint signs of minor disturbance are present, which could be caused by a low mass interaction with a smaller satellite galaxy. Given its overall morphology, the galaxy is likely a relatively massive, evolved system. The object's red color indicates a population of older stars and a lack of significant ongoing star formation.
