The galaxy appears to be a relatively smooth, centrally concentrated system. The light profile suggests a significant bulge component, with the majority of the light emanating from the core. The galaxy exhibits an elliptical morphology, appearing slightly elongated, but generally rounded in shape. There is no prominent spiral structure visible, no strong evidence of dust lanes. The galaxy is yellowish-red in color, indicating an older stellar population and lower ongoing star formation. There are no apparent signs of major mergers or significant tidal disturbances in the galaxy's structure.
