The galaxy appears to be a spiral galaxy, viewed at an angle between face-on and edge-on. There are hints of spiral arm structure in the disk, although the arms are not very well defined. The central bulge appears prominent and exhibits a yellowish hue, possibly indicating an older stellar population. The disk component surrounding the bulge appears bluer, suggesting ongoing star formation. The galaxy has a relatively high degree of central concentration. The overall shape seems somewhat elliptical, although this could be partly due to the viewing angle. There are no obvious signs of a major ongoing merger or strong tidal disturbance, but a minor disturbance cannot be ruled out. A bar feature is not readily apparent. The galaxy is moderately bright.