The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a bright, concentrated core region. The radial light profile appears to decrease smoothly from the center, showing no evidence of prominent spiral arms or significant disk-like features. There are subtle color variations across the galaxy, with a slightly bluer hue in the outer regions, suggestive of some ongoing, albeit low, star formation. The overall color is relatively red, indicating an older stellar population. The galaxy exhibits a high degree of symmetry and roundness. There are no obvious signs of tidal disturbances or major mergers.
