The galaxy appears as an elliptical-like structure with a high degree of central concentration. The light profile suggests a smooth distribution with minimal visible features such as spiral arms or distinct substructures. The galaxy displays a yellowish hue, possibly indicating an older stellar population dominated by evolved stars, with minimal ongoing star formation activity. The overall morphology is consistent with an early-type galaxy, likely an elliptical or lenticular type. There are no signs of significant tidal disturbances or ongoing mergers; the shape is relatively regular, lacking prominent asymmetries or distortions.
