This galaxy appears to be a relatively smooth, elliptical or lenticular type galaxy at a considerable distance. The central bulge is prominent and exhibits a yellowish-orange hue, suggesting a population of older stars. There is little evidence of spiral arms or significant dust lanes. The overall shape is close to round. The galaxy's luminosity indicates it is a massive system. There are no obvious signs of recent major merger activity, although minor disturbances or interactions cannot be ruled out based on the image alone. There is evidence of active star formation.
