The observed galaxy presents as a face-on spiral galaxy, exhibiting a prominent central bulge that appears yellowish in color, suggesting a population of older stars. Faint spiral arms extend outwards from the bulge, though their definition is somewhat indistinct, likely due to the image resolution. The arms display a tightly wound morphology. There is an absence of significant dust lanes or prominent star-forming regions visible within the spiral arms. The overall elliptical shape of the galaxy suggests it is being observed nearly face-on. The low level of distortion suggests the galaxy is not undergoing any major mergers. The galaxy appears relatively isolated. 
