The galaxy appears as a flattened, elongated structure, likely a disk galaxy viewed at a significant inclination. The central bulge region exhibits a yellowish hue, suggesting a population of older, cooler stars. Fainter bluish regions can be observed in the outer disk, potentially indicative of younger, hotter stars and ongoing star formation. There does not appear to be any significant disturbances or tidal features suggesting a recent major merger. The overall morphology suggests a relatively undisturbed disk galaxy with a smooth profile, but subtle disk features may be present. The galaxy's moderate size and low star formation rate indicate a mature system.
