The galaxy presents as a spiral type, exhibiting a prominent disk structure with notable spiral arms. The arms appear tightly wound, suggesting a grand-design spiral galaxy morphology. A central bulge is clearly visible, appearing moderately sized. A bar structure seems to be present, potentially classified as a strong or weak bar based on visual estimation. The overall color of the galaxy leans towards the redder end of the spectrum. There are some merging features, which may indicate ongoing or recent galaxy interactions. The spiral arm count suggests a two-arm system predominates.
