The galaxy presents as a face-on spiral, exhibiting a complex structure with prominent spiral arms. The arms are tightly wound, originating close to the galactic center and extending outwards. The central bulge appears relatively small and faint. The color gradient across the galaxy shows a shift from bluer hues in the spiral arms to slightly redder tones in the central region, possibly indicating variations in stellar populations and dust distribution. There is no clear presence of a strong bar feature bisecting the center of the galaxy. The overall morphology suggests a relatively undisturbed spiral structure, though there appears to be some signs of minor disturbances, such as asymmetries or irregularities in the spiral arm pattern. The galaxy does not appear to be undergoing a major merging event.
