The galaxy appears to be a spiral galaxy, exhibiting a disk-like structure. Distinct spiral arms are visible, winding moderately around the galactic center. The arms appear populated with regions of active star formation, indicated by bluer hues. A central bulge is present, appearing moderately sized, contributing to the overall luminosity of the galaxy. The disk is not perfectly edge-on, providing a clear view of the spiral structure. The galaxy exhibits a lack of significant morphological disturbances or signs of ongoing major mergers.
