The galaxy presents a distinct spiral morphology, exhibiting two prominent spiral arms emanating from a central bulge. The arms are moderately wound and extend outwards, displaying varying degrees of prominence.

The central bulge appears moderate in size. A bar structure appears visible running through the center of the galaxy. The galaxy disk appears oriented close to face-on.

Color gradients suggest active star formation within the spiral arms, particularly in the bluer regions, while the central bulge exhibits a yellower hue, potentially indicating an older stellar population. There is no visually obvious evidence of any major merger. There appears to be a minor disturbance or possibly a merging event occurring on the left side of the galaxy.
