The galaxy presents a clear spiral structure, with two prominent arms emanating from a central bulge. These arms appear tightly wound near the core and gradually loosen as they extend outwards. A stellar bar is also visible, albeit subtle. The bulge is fairly small, with a moderate amount of light concentrated in the galactic center. The arms exhibit a bluish hue, which is indicative of active star formation regions. The central bulge appears more yellow/orange, possibly indicating an older stellar population. The spiral arm structure is well-defined. Overall, this galaxy appears to be a relatively undisturbed spiral, with no obvious signs of a major merger event.
