The galaxy appears to be a spiral galaxy with a relatively smooth, centrally concentrated bulge. The bulge exhibits a yellowish-orange hue, potentially indicating an older stellar population dominated by redder stars. Fainter spiral arms are suggested in the surrounding disk of the galaxy, which display a bluer color, indicating younger stars, perhaps undergoing active star formation. The disk appears moderately inclined with respect to our line of sight. There are also features that could be minor disturbances within the galaxy. The overall shape is somewhat elliptical.
