The galaxy presents as a spiral type, with a prominent central bulge exhibiting a high degree of luminosity. The spiral arms are well-defined, although moderately flocculent in nature, displaying a winding structure which would be categorized as intermediate. Two dominant spiral arms appear most prominent, with evidence of fainter, branching arms also detectable. The arms exhibit a bluer coloration than the central bulge, suggestive of ongoing star formation within these regions. The galaxy exhibits a slight degree of asymmetry, with a possible minor interaction or tidal disturbance observable in the morphology of the arms. The bar is weakly apparent. No strong evidence of a recent or ongoing major merger is apparent, although there may be minor distortions. The disk appears relatively flattened.