The galaxy exhibits a flattened, disk-like morphology observed edge-on. The central bulge region appears prominent and concentrated, displaying a yellowish-white hue suggestive of an older stellar population. The disk component is fainter and extends outward from the bulge, showing subtle color variations with hints of blue along the edges. These colors imply the presence of younger, hotter stars in the disk, although star formation activity seems relatively low. No significant signs of spiral arm structure or active galactic nuclei are visibly discernible in the image. Overall, the galaxy appears to be a relatively undisturbed system, showing signs of being a smooth disk galaxy. No significant tidal distortions or indications of major mergers are apparent.
