The galaxy appears as an elliptical structure, showing a smooth, centrally concentrated light distribution. It displays a subtle color gradient, transitioning from a yellowish core to a slightly redder outer region. The galaxy appears moderately luminous. The overall shape is somewhat elongated, with a slight deviation from a perfect circular form. The edges of the galaxy seem diffuse, lacking sharp boundaries, which suggests a gradual decrease in stellar density. There is no obvious presence of spiral arms, dust lanes, or other distinct morphological features typically associated with disk galaxies. The galaxy shows little sign of recent mergers.
