The galaxy presents as a spiral type, displaying a prominent disk structure. The spiral arms are somewhat tightly wound around the central bulge, with suggestions of several arms extending outwards. The bulge appears moderately sized and exhibits a yellowish hue, indicative of an older stellar population. The disk shows a bluer coloration, likely due to the presence of younger, hotter stars and ongoing star formation. There is evidence of some dust lanes within the spiral arms. Overall, the galaxy seems relatively undisturbed, displaying a classic spiral morphology without obvious signs of a major merger, though some minor gravitational interaction cannot be ruled out.
