The galaxy appears to be a relatively smooth, centrally concentrated object. The light distribution suggests a bulge-dominated morphology. The galaxy exhibits a generally elliptical shape, with a hint of deviation from perfect circularity. The color gradient suggests a radial change in stellar population, with a bluer inner region and redder outer regions. There is no discernible evidence of spiral arms or significant tidal disturbances. The overall structure indicates a relatively undisturbed system, potentially an early-type galaxy.
