The galaxy presents as an elliptical or lenticular type, exhibiting a smooth, relatively featureless morphology. There is little or no visible dust or spiral arm structure. The light profile is highly concentrated towards the center, suggesting an older stellar population. The galaxy displays a generally round shape. There is no obvious tidal disturbance or other clear indication of recent or ongoing merger activity. The galaxy color appears to be slightly redder in overall color, consistent with a population of older, cooler stars and a low rate of star formation.
