This galaxy presents as a spiral galaxy with a notable disk structure. The spiral arms are fairly well-defined, though somewhat patchy. The galaxy exhibits a prominent central bulge. The bulge appears yellow-white, suggesting a population of older stars. The disk shows a bluer hue, likely due to ongoing star formation. The galaxy is not perfectly symmetrical; there may be some minor tidal distortions or interactions with other galaxies in its environment. Overall, the galaxy is a relatively typical spiral with a moderate bulge and active star formation within its disk.
