This galaxy presents a distinct spiral structure. The arms are well-defined, exhibiting a grand design morphology. The winding of the spiral arms appears moderately tight in some regions and more open in others. The central bulge is elongated, suggesting the presence of a bar structure. The bar extends through a significant portion of the galaxy's central region. The disk appears relatively thin and is viewed close to face-on. Patches of blue indicate regions of active star formation within the spiral arms. The overall color of the galaxy suggests a mix of stellar populations, with older, redder stars concentrated towards the bulge and younger, bluer stars populating the spiral arms. There are no readily apparent signs of major merger activity, although minor asymmetries or disturbances cannot be ruled out without further investigation.
