This galaxy presents a clear spiral structure, although the arms are somewhat flocculent. It appears face-on relative to our line of sight. Two distinct spiral arms are prominently visible, exhibiting a moderate degree of winding, as they curve out from the central bulge. The arms display regions of concentrated star formation, indicated by their bluer hue.

The central bulge presents a moderate size compared to the overall galaxy disk, and exhibits a yellowish-white color gradient. The bulge appears slightly elongated, suggesting the possible presence of a bar structure, though it is not exceptionally prominent. There is no visual evidence of a recent major merger event disrupting the overall morphology of the galaxy. A minor irregularity appears in one of the arms, potentially indicative of a minor gravitational interaction or internal dynamic process.
