The galaxy appears to be a spiral galaxy, observed at an intermediate inclination angle relative to our line of sight.  A distinct central bulge, yellowish-orange in color, is evident, suggesting an older stellar population concentrated towards the galaxy's core.  Fainter, bluer spiral arms extend outward from the bulge, indicating the presence of younger stars and ongoing star formation. The spiral arms are tightly wound, showing a high degree of organization. There is a hint of a bar-like structure running through the center of the bulge along the major axis.  The disk appears to be quite extended with a non-negligible radius.  The presence of dust lanes may be obscuring some of the starlight within the disk. The overall morphology suggests that the galaxy is relatively unperturbed with no major ongoing mergers.
