The object appears to be a relatively smooth galaxy, exhibiting a generally elliptical morphology. It presents with a concentrated central bulge, which appears yellowish-white, indicative of an older stellar population. The outer regions display a slight decrease in intensity, showing a gradual fading. There may be subtle hints of a disk structure. This object is likely a galaxy with a substantial spheroidal component. No clear signs of recent mergers or major disturbances are observed. There is a slight green hue around the yellow center, possibly indicating recent star formation.