This galaxy appears to be a spiral galaxy viewed at a significant inclination. It presents a flattened, disc-like structure with a prominent central bulge. The bulge exhibits a yellow-orange hue, possibly indicative of an older stellar population. Surrounding the bulge, the disk shows hints of spiral arm structure, which appear somewhat indistinct and patchy. These spiral arms show hints of blue-green regions, potentially signifying areas of ongoing star formation. Overall, the galaxy displays a relatively smooth texture, with only minor irregularities or disturbances visible in its morphology. It does not appear to be undergoing a major merging event. The color gradients suggest a mix of stellar populations, with older stars concentrated in the bulge and younger, hotter stars distributed throughout the disk.
