The galaxy presents as a relatively face-on spiral, though the spiral structure appears somewhat indistinct. The central bulge is bright and elliptical, with a yellowish-white hue, suggesting a significant population of older stars. The disk surrounding the bulge exhibits a bluer color, indicative of ongoing star formation. The disk appears to be slightly disturbed, possibly indicating a minor interaction or merger event. There may be some tidal features that are close to the galaxy itself. It is an overall average spiral galaxy, and there is nothing that makes it too distinct from other similar galaxies.
