The galaxy presents as a spiral structure with a centrally concentrated bulge. Two dominant spiral arms are visible, exhibiting a relatively tight winding pattern around the galactic center. The arms show subtle color variations, suggesting ongoing star formation. The orientation is roughly face-on. There appears to be a moderate bulge. There are some minor disturbances. The central bulge displays a yellowish hue, while the spiral arms show a bluer tint, indicative of younger stellar populations.
