The galaxy presents as a centrally concentrated, relatively smooth object. Its overall color appears to be a pale blue-white, indicative of a moderate population of young, hot stars. The light is somewhat diffuse, suggesting a lack of strong spiral arm structure or prominent dust lanes. The morphology indicates the galaxy is likely an early-type spiral galaxy, with a dominant bulge and a tightly wound disk. The slight ellipticity suggests the galaxy is inclined somewhat relative to our line of sight. There is no apparent sign of active galactic nuclei or ongoing major mergers.
