The galaxy presents a clear spiral structure, with two prominent spiral arms that emanate from a moderately sized central bulge. The spiral arms are relatively tightly wound around the galactic center. The overall color of the galaxy appears to be a blend of yellow and blue, with the central bulge exhibiting a warmer, more yellow hue, suggesting an older stellar population. The spiral arms show bluer regions, indicative of ongoing star formation. There is a hint of a central bar that appears to run through the bulge region, potentially influencing the spiral arm structure. The disk of the galaxy is viewed at an angle that is not quite edge-on, allowing the spiral structure to be discerned, but some of the finer details are obscured by the viewing angle. There are no obvious signs of a recent major merger. It is possible that there are some minor tidal disturbances or smaller galaxies merging with it.