The galaxy presents as a centrally concentrated object with a smooth light distribution, exhibiting an elliptical morphology. The core region is bright and appears yellowish. Moving outwards, the color gradient indicates a possible transition to slightly redder hues in the outer regions, though this is subtle. No distinct spiral arms or bar structures are visible, suggesting it could be an early-type galaxy. There is no strong evidence of tidal disturbances or ongoing major mergers, although the galaxy appears not perfectly spherical in shape. The absence of prominent blue regions suggests a relatively low rate of current star formation activity. The overall appearance points toward a galaxy dominated by an older stellar population.
