The galaxy appears as a centrally concentrated, elliptical structure with a smooth light distribution. Its color suggests a predominantly older stellar population, with a yellow-red hue dominating the galaxy's core and outskirts. The isophotes appear elongated, indicating a non-circular shape. There is no visible evidence of spiral arms, dust lanes, or active star formation regions. The smooth light profile suggests a relatively quiescent galaxy, likely an elliptical galaxy that has largely exhausted its gas supply.
