The galaxy presents a notable spiral structure. Two spiral arms are clearly visible, exhibiting a winding pattern that transitions from moderately tight near the core to looser at the periphery. The arms appear to be fairly symmetrical. The central bulge is prominent, with a moderate size relative to the overall galactic disk. The bulge displays a smooth, yellowish color, indicative of an older stellar population. The disk exhibits a bluer hue, suggesting ongoing star formation. There is no strong evidence of a central bar structure. Minimal signs of significant tidal disturbances or interactions with other galaxies are apparent; there are no obvious signs of a major ongoing merger event. The overall morphology leans towards a classic spiral galaxy, with a well-defined disk and bulge component.
