The galaxy presents as a flattened, disk-like structure, viewed at an oblique angle. The central region appears brighter and more yellow-white in color, indicative of an older stellar population. A distinct ring-like feature surrounds the central bulge, exhibiting a bluer hue, suggesting active star formation. This ring is not perfectly uniform, with some areas appearing more prominent than others. The outer edges of the galaxy fade gradually into the background, without any clear spiral arm structure or tidal features visible. Overall, the morphology suggests a galaxy with a dominant central bulge surrounded by a disk and a prominent star-forming ring. The smoothness of the overall light distribution indicates a relatively undisturbed system, with perhaps only minor past interactions.
