This galaxy exhibits a distinct disk-like structure, viewed nearly edge-on from our line of sight. The central bulge appears prominent and elongated, indicating a potentially bar-shaped morphology. The bulge presents a noticeable yellow-orange hue, which may be indicative of an older stellar population dominating this region. The disk exhibits a bluer coloration especially towards its periphery, suggestive of more recent star formation activity. Some areas of the disk demonstrate mottling which may suggest dust obscuration. The disk shows a relatively undisturbed morphology; tidal tails or other signs of recent major mergers are not apparent, suggesting a relatively isolated system.
