The galaxy presents as a single, relatively smooth, elliptical object. Its overall color is yellowish, indicating a dominant population of older stars, with potentially low current star formation. The galaxy exhibits a high degree of central concentration of light, with a gradual decrease in surface brightness towards the outer regions, which suggests a bulge-dominated morphology. The round shape and lack of clear spiral arm structures further support the classification as an elliptical galaxy. There is a slightly brighter, less concentrated object that could be an interaction with another galaxy. There's a potential for the galaxy to be undergoing a merger or interaction, however, further data would be needed to fully assess this interaction.
