The galaxy presents as a relatively face-on spiral, although the spiral arms are not sharply defined, appearing somewhat flocculent. The central bulge is prominent and concentrated, exhibiting a yellowish hue suggesting an older stellar population. The disk component shows a bluer tint, indicative of younger stars and ongoing star formation, albeit at a lower rate. There is a slight elongation to the galaxy's shape, deviating from a perfect circular profile. The overall structure appears relatively undisturbed, showing no strong signs of major mergers or tidal interactions.