This galaxy appears to be a spiral galaxy, viewed nearly edge-on from our perspective. A prominent dust lane bisects the galaxy's disk, obscuring the light from stars behind it. The central bulge appears relatively large and smoothly distributed in brightness, indicative of an older stellar population. The disk appears to be a yellowish orange, which could suggest older stars or a significant amount of dust. The shape of the bulge is quite rounded. There is no apparent sign of merging or major disturbances.