The galaxy presents as an elliptical or lenticular type, exhibiting a smooth, largely featureless morphology with a high degree of central concentration. The core region is bright and intensely luminous, suggesting a significant density of stars. The light profile appears to decrease gradually from the center outwards, lacking prominent spiral arms or strong dust lane features.

The overall color index implies a relatively old stellar population, as the galaxy exhibits a reddish-yellow hue. This suggests a lower rate of ongoing star formation. There may be a smaller concentration of light visible in the galaxy to the bottom-right of the core.

The general symmetry suggests a settled system without obvious signs of recent major mergers or tidal disturbances. Any subtle interactions or minor disturbances would require deeper imaging and analysis to confirm. Overall, the galaxy appears to be a well-formed system.
