The galaxy presents as a well-defined spiral galaxy, observed at a near face-on orientation. A prominent central bulge appears bright and concentrated, exhibiting a yellowish-white hue suggesting an older stellar population. Two main spiral arms emanate from the central bulge, and wind around the galaxy. The arms appear to be flocculent, with numerous star-forming regions visible as bluish-white knots embedded within the arms. The disk of the galaxy appears smooth with a bar in the center, while dust lanes are also subtly interspersed throughout the arms, contributing to the galaxy's overall structure. The galaxy displays a classic spiral morphology with a clear separation between the bulge and the disk components. The disk extends to a radius of approximately 4 kiloparsecs. A very weak sign of a merger or minor disturbance can be seen with slight differences in each spiral arm.
