The galaxy presents as a slightly inclined disk galaxy, though the features are somewhat muted. The central bulge appears relatively smooth and diffuse. The spiral arms are not well-defined, showing more as subtle variations in luminosity and color, without distinct arm structures. There's a hint of bluer regions within the disk, indicating areas of potential star formation, but these are not prominent. Overall, the galaxy's light distribution suggests a system with a relatively even distribution of stars, with ongoing, but not highly active, star formation. The galaxy's apparent roundness suggests it could be closer to face-on. There is no obvious indication of any major ongoing mergers, though there may be some minor disturbances within the disk.
