The galaxy appears as a single, relatively smooth object. Its light is concentrated towards the center, with a gradual decrease in brightness moving outwards, suggesting a high degree of central mass concentration. There are no distinct spiral arms or obvious dust lanes visible in the image. The galaxy exhibits a generally elliptical shape with a high degree of roundness. There are no readily apparent signs of ongoing major mergers or significant tidal disturbances, though minor disturbances cannot be ruled out. The color profile shifts from a yellowish-white core to reddish hues in the outskirts. This color gradient implies an older stellar population in the outer regions of the galaxy.
