The galaxy exhibits a spiral structure, viewed at a slight angle, but not perfectly edge-on. The disk shows prominent spiral arms that appear somewhat tightly wound in some regions and looser in others. While the structure is apparent, the resolution makes it difficult to discern fine details. The central bulge appears moderately sized and a yellowish color, suggesting an older stellar population. Fainter, bluer regions within the spiral arms suggest areas of more recent star formation. There appears to be a weak bar structure present. The overall morphology indicates a relatively undisturbed system, with no obvious signs of a major merger, though minor disturbances cannot be ruled out. The luminosity appears to be quite high, indicating a substantial stellar mass.
