The galaxy presents as a spiral structure with a prominent, moderately sized bulge at its center. Spiral arms are distinctly visible, exhibiting a tightly wound morphology. The color distribution suggests ongoing star formation within the arms, indicated by the bluish hues. The bulge appears more yellow, potentially indicative of an older stellar population. There are no strong indications of a bar structure. Based on visual inspection, the galaxy appears relatively undisturbed, showing no immediately apparent signs of a major merger event. Some tidal disturbances may be present, but the system is largely intact.
