The galaxy presents as a fairly bright, centrally concentrated object. It appears largely featureless and smooth in texture, with a generally elliptical morphology. The core region is noticeably brighter and yellower compared to the outer regions, suggesting an older stellar population concentrated towards the center. The outer halo appears more diffuse and somewhat redder in color, which is characteristic of a galaxy with minimal ongoing star formation. There is a hint of asymmetry in the light distribution of the outer regions, but no strong evidence of tidal tails or significant disturbances indicating a recent major merger event.
