This galaxy presents as a grand design spiral, possessing a disk-dominated morphology.  The spiral arms are well-defined, extending from a central bulge of moderate size. The winding of the spiral arms appears to be predominately tight to medium.  The galaxy exhibits a notable degree of star formation activity, indicated by the presence of some blue regions within the spiral arms. There is no visual evidence of a strong bar structure bisecting the central bulge.  The overall structure does not appear to be significantly disturbed, though some minor tidal features cannot be ruled out.  The color gradient suggests a radial distribution of stellar populations, with older, redder stars concentrated within the bulge, and younger, bluer stars prominent in the spiral arms.
