The galaxy presents as a largely featureless, elliptical-like form with a concentrated central bulge. The light is fairly smooth and diffuse. The galaxy exhibits a predominantly yellow-orange hue, which may indicate an older stellar population. There is very little evidence of dust lanes, spiral arm structures, or active star formation regions within this image. The galaxy appears quite round, showing no strong signs of tidal disruption or ongoing merger activity. Overall, the morphology suggests an evolved system with minimal ongoing star formation.
