The galaxy presents as a spiral type, observed at an oblique angle, revealing a flattened disk-like structure. A central bulge is prominent, exhibiting a bright, concentrated luminosity. The spiral arms are well-defined. The arms are tightly wound, with the dominant arm count of two, though this is not perfectly discernible. Evident dust lanes are observed. There is a strong bar structure present. No major mergers are taking place. The galaxy displays a relatively small bulge size, indicating a disk-dominated morphology.