This galaxy presents as a spiral galaxy with a distinct disk structure. The spiral arms are prominent, displaying a moderately loose winding pattern. Two main spiral arms are clearly visible. A central bar structure appears to traverse the galactic nucleus. The bulge is of small to moderate size. Some signs of disturbances are observed, but no major merging is apparent. The color distribution suggests active star formation occurring within the spiral arms, indicated by the bluer hues. The central region has a slight reddening, possibly indicating older stellar populations and dust.
