This galaxy appears to be a disk galaxy, observed at an angle. The central bulge is bright and concentrated, with a near-white color, suggesting a population of older stars. A ring-like structure with a greenish-blue hue surrounds the central bulge, indicating regions of active star formation. Fainter, diffuse redder material is evident within and surrounding the bluish band. The overall morphology does not suggest a recent major merger, but some slight asymmetries might indicate minor interactions or internal disturbances. The galaxy appears relatively compact.
