The galaxy presents as a spiral with a relatively bright, moderately sized central bulge. The spiral arms are well-defined, exhibiting a multi-armed structure, and appear somewhat tightly wound closer to the center but begin to wind more loosely as they extend away from the central region. The disk is viewed nearly face-on, revealing detailed structure within the arms. Patchy regions of star formation are visible along the spiral arms as a slightly bluer coloration than the rest of the disk. There is evidence of a bar structure transecting the central bulge, but this bar is more of a modest structure within the galaxy. There are no obvious signs of major tidal disturbances or interactions with other galaxies.
