The galaxy presents as a spiral type, exhibiting a prominent disk structure. Its orientation is presented in a face-on manner. Two spiral arms are distinctly visible, winding moderately from the central bulge. The nucleus is bright and slightly elongated, potentially indicating a weak bar structure. The bulge appears relatively small. Patches of blue color are visible within the spiral arms, indicative of ongoing star formation regions. There is no evident major disturbance to the morphology, which suggests no recent major merger event. There is some evidence of a minor disturbance.
