The galaxy presents as a disk galaxy, viewed at an oblique angle, somewhere between face-on and edge-on. A prominent central bulge is visible, exhibiting a concentrated luminosity profile. The bulge appears to be approximately 1/3rd of the overall diameter of the galaxy. A faint disk surrounds this central bulge. This disk appears smooth, indicating it is largely composed of older stars. The light distribution is relatively uniform, lacking strong spiral arm structures or prominent dust lanes. The galaxy exhibits a moderately elliptical shape, and appears to be relatively large. Overall, the galaxy has a somewhat muted color profile.
