The galaxy presents a notable disk structure, tilted somewhat away from an edge-on orientation. The galaxy exhibits clear spiral arm morphology. Evident is a distinct central bulge region, accounting for a moderate fraction of the overall galactic light. A bar-like structure appears to transect the bulge. There are no signs of major mergers. The galactic light is extended. There is a large degree of concentration in the R-band, with the galaxy appearing brighter in the redder bands, suggesting an older stellar population.
