The galaxy presents as a centrally concentrated, largely featureless system. Its overall morphology appears elliptical or spheroidal. The light distribution suggests a smooth profile with a dominant central bulge that fades gradually outward. The color appears yellowish-white, suggesting an older stellar population. There's minimal evidence of dust lanes or spiral arm structures. The galaxy is relatively isolated with no immediately apparent signs of tidal interaction or ongoing merger activity. Overall, the galaxy appears to be a relatively quiescent system that is round. 
