This galaxy exhibits a flattened, disk-like morphology. The central region appears bright and concentrated, with a yellowish hue, suggesting an older stellar population. Moving outwards from the core, a distinct ring-like structure is visible. This ring displays variations in color, with regions showing bluer tones, which could indicate areas of active star formation. The outer regions of the galaxy appear fainter and more diffuse. The overall smoothness suggests a lack of significant spiral arm structure. There is a faint asymmetry in the light distribution, potentially indicating minor gravitational interactions or disturbances. Though largely smooth, some subtle features are present that may indicate minor disturbances. No prominent tidal tails or signs of recent major merger activity are apparent in this image.
