The galaxy exhibits a clear spiral structure. The spiral arms are well-defined, with a relatively tightly wound morphology in the inner regions transitioning to a more open, medium winding in the outer parts. At least two spiral arms are clearly visible, potentially with hints of additional arm segments.

The central bulge appears prominent, exhibiting a yellow/orange hue, suggesting an older stellar population. The disk surrounding the bulge shows a bluer coloration, potentially indicating ongoing star formation activity within the spiral arms. The central region hosts a strong bar, that spans the majority of the radius.

There are possible signs of minor disturbances, or perhaps ongoing interactions with smaller satellite galaxies, but its main classification is that of a spiral galaxy. The overall color suggests a combination of evolved stellar populations and more recent star formation.
