The galaxy presents a clear spiral structure, oriented somewhat face-on relative to our line of sight. The spiral arms appear tightly wound, tracing a relatively smooth pattern throughout the disk. The central bulge region is prominent and appears to be of moderate size. There is an indication of a bar structure running through the core of the galaxy. The disk is bluer in color than the bulge, suggesting a relatively active star formation in the disk. The presence of a weak or moderate bar could be influencing star formation in the central region. Based on its shape and the presence of spiral arms, the galaxy appears to be a late-type spiral. There are no obvious signs of major tidal disturbances or ongoing mergers, although minor disturbances can not be ruled out. The galaxy appears relatively isolated.
