The galaxy appears to be a relatively face-on spiral, though the resolution limits detailed observation. The central bulge exhibits a yellowish hue, indicative of an older stellar population. Fainter spiral arms can be discerned extending from the bulge, showing hints of bluer regions, possibly regions of more recent star formation. The galaxy seems to be relatively undisturbed, showing only slight asymmetry and no apparent signs of a major merger. It appears to be a disk galaxy that is fairly smooth, but slightly elongated.
