The galaxy presents as a spiral structure, exhibiting a notable disk component and a distinct central bulge. The spiral arms are prominent, displaying a loosely wound morphology and appear to have a dominant two-arm structure. There is evidence of ongoing star formation, indicated by the blue hue within the spiral arms. The central bulge appears moderately sized relative to the disk, and exhibits a yellow-reddish color, suggesting a population of older stars. Faint dust lanes might be present within the spiral arms. There is some evidence of a bar-like structure. The galaxy overall appears to be relatively undisturbed, with only hints of minor disturbances potentially indicating minor interactions or mergers.
