This galaxy appears to be a relatively smooth, elliptical system. Its central region exhibits a concentrated, reddish-orange hue, indicative of an older stellar population. The galaxy's overall shape is approximately round with a slight elongation, hinting at a possible departure from perfect sphericity. There is a noticeable color gradient from the center outwards, with the outer regions displaying a greener tinge, which could suggest the presence of some younger stars or a different chemical composition in the outer halo. No distinct spiral arms or prominent dust lanes are discernible, further supporting its classification as an elliptical or lenticular galaxy. There is no obvious visual evidence of any major ongoing merger activity or significant tidal disturbances.
