The galaxy presents as an inclined spiral with a prominent central bulge, exhibiting a moderate degree of concentration. A well-defined disk surrounds the central bulge, appearing relatively smooth with hints of arm structure that are difficult to resolve distinctly. The dust lanes are subtle. Color gradients suggest a presence of older stellar populations throughout the bulge and inner disk, with bluer colors associated with star formation in the outer regions of the disk. The morphological classification indicates a moderate bulge size. There appears to be no obvious interaction or signs of a major merger event in the recent past. The overall structure reveals a barred morphology, which may contribute to gas inflow towards the center. The relative smoothness and lack of prominent star-forming knots imply a gradual star formation rate distributed throughout the disk.
