The galaxy presents a face-on spiral structure. The central bulge is prominent and appears relatively smooth and yellow-white in color, suggesting an older stellar population. Two dominant spiral arms extend outwards from the central bulge, exhibiting a moderately wound morphology. The arms show hints of blue color, indicating the presence of younger, hotter stars and ongoing star formation. There is a suggestion of bar structure within the central bulge. The disk exhibits intermediate brightness, and the overall structure appears relatively undisturbed, lacking any major signs of ongoing mergers or tidal disruptions.
