The observed galaxy presents a notable disk-like morphology, viewed at a high inclination, approaching an edge-on orientation. The central bulge is prominent, exhibiting a yellowish hue, potentially indicative of an older stellar population. Fainter, bluer regions, suggesting more recent star formation, are visible within the disk, extending outward from the bulge. Evidence of spiral arm structure is present, however due to the viewing angle and blurring effects it is not clearly defined. There are no other objects in this image which appear to show signs of disturbance or merging.