The galaxy appears as a flattened, disk-like structure, viewed nearly edge-on. A prominent central bulge is not readily apparent; however, an area of increased light concentration near the central region is visible. The disk exhibits a blue hue, suggesting the presence of younger stellar populations and ongoing star formation. Two distinct pinkish-red regions are visible in the disk, aligned parallel to the central region, potentially indicative of HII regions or areas of intense star formation. The galaxy displays a degree of smoothness in its overall structure, with no obvious signs of a major merger or significant tidal disturbances. The overall morphology suggests a relatively undisturbed disk galaxy, likely undergoing active star formation within its disk.
