The galaxy appears to be a spiral galaxy with a smooth structure. It exhibits a slight elongation, with a noticeable bulge at its center. The bulge has a yellowish-orange hue, suggesting an older stellar population, while the surrounding disk shows faint blue tinges, potentially indicating younger stars and ongoing star formation. The disk appears disturbed with signs of tidal interactions or a possible minor merger. There are faint, elongated features extending from the main body of the galaxy that could be tidal tails.
