The galaxy presents a prominent, centrally concentrated bulge. Faint, loosely wound spiral arms extend outwards from the central region, tracing a relatively smooth path. A possible weak bar structure may be present within the central region. The disk appears to be viewed at a slight angle, but is nearly face-on. There is no evidence of any major mergers or significant tidal disturbances to the main galactic structure. The color of the galaxy is largely consistent with a relatively high star formation rate.
