The galaxy appears to be a relatively smooth, elliptical or lenticular galaxy. It exhibits a concentrated central bulge that is yellowish in color, suggesting a population of older stars. The overall shape is generally round. There's a hint of a very faint, greenish disk component extending asymmetrically from one side of the central region, suggesting possible recent star formation in this area. The galaxy does not show obvious signs of major mergers or significant tidal disturbances, though there may be some minor perturbation in the asymmetry of the green disk. Overall, it seems to be a reasonably evolved galaxy, likely of substantial mass, with a dominant old stellar population and perhaps a small ongoing component of star formation.
