This galaxy exhibits a distinct spiral structure with well-defined arms. These arms appear somewhat flocculent, not tightly wound. The central bulge is relatively small to moderate in size, presenting a smooth, concentrated brightness. There is a hint of a bar-like structure across the center, though it is not prominently defined. The galaxy's color profile indicates the presence of both older stellar populations in the bulge, exhibiting a yellow hue, and younger, bluer stars scattered throughout the spiral arms. The disk component appears dominant and does not seem to be disturbed by any major merging events. The object is not viewed edge-on.
