The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. There is a slight elongation in its shape, but it is generally rounded. The central region exhibits a yellowish hue, likely indicating an older stellar population. Fainter, reddish outer regions suggest the presence of some dust or a cooler population of red giant stars. There's no strong evidence of spiral arms or significant star formation activity visible in the image, although a very small amount may be occurring. The overall structure indicates it's a well-formed and relatively undisturbed system, not currently undergoing major merger events.