The galaxy appears to be a spiral galaxy, observed at a low inclination angle. There is a bright, concentrated central bulge. It seems to have a relatively smooth appearance, with a higher concentration of older stellar populations. The spiral arms appear somewhat faint and tightly wound, showing bluer hues indicating some ongoing star formation, though not dominant. The galaxy's overall color suggests it has passed its peak star-forming epoch. There is no obvious signs of a major merger event. There are some features that suggest a minor disturbance or interaction. The galaxy exhibits a degree of roundness and symmetry in its overall morphology. 
