The galaxy presents a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge that gradually fades into an extended halo. The color profile suggests a dominant population of older stars, with a reddish-orange hue prominent throughout the structure, indicating minimal ongoing star formation. There is a possible minor disturbance of asymmetry in the shape, suggesting that the galaxy could be undergoing, or have recently undergone a minor interaction, or merger with another galaxy. No distinct spiral arms or prominent dust lanes are visible.
