The galaxy presents as a spiral type, exhibiting prominent, well-defined arms. It is not seen edge-on. The spiral arms have a clear winding structure. A strong presence of two spiral arms are observed. The nucleus appears as a centrally concentrated bulge of moderate size, characterized by a bright, yellowish hue, with a slight color difference in comparison to the rest of the disk. There is a suggestion of a bar-like structure. The overall morphology is suggestive of ongoing star formation, which accounts for the blue hue in parts of the arms. The galaxy displays a generally symmetric structure. There are hints of some minor disturbance in the shape.
