This galaxy exhibits a clear spiral structure, with tightly wound arms emanating from a central bulge. The arms are well-defined, with noticeable concentrations of star formation regions. The color gradient across the galaxy suggests differing stellar populations, with a redder core indicating older stars and bluer arms indicating more recent star formation. There appears to be a bar-like structure extending through the center of the galaxy. There are no signs of major mergers but there are small disturbances in the disk. The galaxy displays a moderate inclination with respect to our line of sight.
