The galaxy appears to be a spiral, seen at an angle between face-on and edge-on. The central bulge is prominent and yellowish in color, suggesting a population of older stars. Fainter spiral arms extend from the bulge, exhibiting a bluer hue, indicative of more recent star formation. The disk appears relatively smooth and featureless. There does not appear to be any merger activity. The galaxy is moderately sized and generally symmetric in structure.
