The galaxy appears to be a relatively smooth, elliptical or lenticular galaxy. Its overall shape is quite rounded, with no apparent significant distortions or tidal features suggesting a recent major merger event. The central region exhibits a yellowish hue, possibly indicating an older stellar population dominating the core. Fainter, somewhat greener emissions are present on one side of the central bulge, which could potentially indicate ongoing, though modest, star formation regions within a disk component. There's no obvious spiral arm structure, and the overall appearance is relatively homogenous, with no prominent dust lanes or regions of intense star formation readily visible. The galaxy is relatively compact.
