The galaxy presents as an elliptical structure with a high degree of central concentration. The light distribution is largely smooth and centrally symmetric. There is no apparent spiral arm structure or prominent dust lanes within the visible light range.

The galaxy exhibits a color gradient, transitioning from a slightly redder core to bluer outer regions. The overall color suggests a population of intermediate to old stars, although the bluer regions indicate the possibility of some ongoing, albeit limited, star formation. The pronounced central concentration suggests a relatively high stellar mass. There are no signs of recent or ongoing major mergers or tidal interactions, suggesting a quiescent evolutionary history. Minor disturbances cannot be ruled out with this image, but the overall morphology points to a relaxed system.
