The galaxy appears as a singular, centrally concentrated object with a relatively smooth, amorphous morphology. It exhibits a generally elliptical shape with a high degree of roundness. There is no apparent substructure such as spiral arms or a distinct galactic bar. The light distribution suggests a dominant bulge component. The color appears slightly redder, indicative of an older stellar population and a lower rate of ongoing star formation. No significant signs of tidal disturbances, close companions, or merger activity are visible.
