The observed galaxy exhibits a distinct disk morphology, viewed at a moderate inclination. Spiral arm structures are clearly visible, displaying a relatively tightly wound pattern. The central bulge appears to be of moderate size, with a yellowish hue suggesting an older stellar population. The spiral arms exhibit a bluer color, indicating ongoing star formation. No signs of major mergers are apparent, although some minor disturbances might be present in the outer regions of the disk. The overall structure suggests a relatively undisturbed spiral galaxy with a well-defined disk and bulge.
