This galaxy presents as a relatively smooth, centrally concentrated object, with a spheroid shape, indicative of an elliptical or lenticular galaxy. The core region exhibits a bright, yellowish-white luminosity, suggesting a high density of older stellar populations and potentially a supermassive black hole actively accreting material. There is no apparent spiral arm structure or distinct dust lanes, further supporting an early-type galaxy classification. The overall color is slightly redder, possibly indicating a lack of significant ongoing star formation. The outer regions of the galaxy appear to fade gradually into the background sky, lacking sharp boundaries. Overall, it seems this galaxy has an organized structure, being more smooth than featured.
