The galaxy presents as a spiral type, exhibiting prominent, well-defined spiral arms extending from a noticeable central bulge. The arms appear somewhat flocculent, displaying a patchy distribution of star-forming regions. There is evidence of ongoing star formation within the arms, indicated by the presence of blueish regions. The central bulge appears relatively smooth and concentrated, suggesting a significant population of older stars. The galaxy is not perfectly face-on, showing a slight inclination relative to our line of sight. Overall, the galaxy appears relatively undisturbed, with no obvious signs of a recent major merger.
