The galaxy presents as a spiral type, exhibiting a defined disk structure. Spiral arms are clearly discernible, demonstrating a relatively tightly wound morphology. The central bulge is moderate in size, displaying a yellowish hue indicative of an older stellar population. While a bar feature appears present, it seems to be of moderate strength. Star formation regions, traced by faint blue hues, are observed along the spiral arms, suggesting ongoing stellar birth. The galaxy appears relatively isolated, without obvious signs of recent major mergers or significant tidal disturbances, although a minor interaction cannot be ruled out. The overall structure suggests a relatively undisturbed, mature spiral galaxy undergoing typical star formation processes.
