The galaxy presents as a disk-shaped system, observed at an intermediate angle, neither perfectly face-on nor edge-on. A central bulge is clearly visible, exhibiting a concentrated, yellow-hued luminosity, indicative of an older stellar population. Extending outwards from the central bulge are fainter, blue-tinged spiral arm structures. These arms appear somewhat diffuse and less tightly wound, suggesting a flocculent spiral morphology. One arm is more pronounced on one side of the galaxy, while the opposite side appears fainter and less defined. The galaxy shows a mild asymmetry, with some signs of disturbance in the outer disk, but the overall structure remains largely intact.
