The galaxy appears to be a spiral galaxy, viewed nearly edge-on. There's a prominent, relatively thin disk structure. Dust lanes are subtly visible as darker, obscuring bands within the disk. The central bulge is not particularly pronounced. There is some evidence of recent or ongoing star formation with faint blueish hints present throughout the disk. The spiral arms are not clearly defined, likely due to the near edge-on viewing angle. There's no significant morphological disturbance, and the galaxy appears relatively isolated, exhibiting no immediate signs of a major merger. However, there may be some minor irregularities in the disk suggesting some sort of gravitational interaction. The low star formation suggests an older stellar population.
