The observed galaxy presents a flattened, disk-like morphology with a prominent central bulge. The galaxy is oriented nearly edge-on to our line of sight. Spiral arm structures are faintly discernible, with indications of ongoing star formation. The central bulge appears relatively smooth, suggesting an older stellar population. The disk exhibits a bluer hue compared to the bulge, consistent with the presence of younger, hotter stars in the spiral arms. There appears to be a slight warp in the disk. The overall structure is well-defined.
