The galaxy presents as a flattened, disk-like structure observed at an oblique angle, appearing nearly edge-on. Its central region exhibits a concentration of light, suggesting a bulge, and a distinct yellow-ish hue. The outer disk displays a bluer color, potentially indicative of younger stellar populations and ongoing star formation, though it's important to note that this is just an estimation based on the image. A dust lane may be obscuring the disk. Overall, the galaxy's shape is somewhat irregular. There is no visual evidence of significant tidal disturbances or a prominent bar structure. Further spectroscopic analysis would be required to confirm any potential interactions or internal dynamics.
