This galaxy appears to be a spiral galaxy viewed at an oblique angle, presenting a somewhat edge-on perspective. There is evidence of a central bulge region which exhibits a concentrated, yellowish-white luminosity, suggesting a population of older, evolved stars. Fainter bluish hues extend from the central bulge, indicating the presence of younger, hotter stars and likely ongoing star formation within the spiral arms. While the spiral arms are not sharply defined, there are indications of a disk-like structure. The overall morphology suggests a galaxy with a disk component, but it's hard to determine any disturbances. The disk also appears relatively smooth, rather than clumpy and disturbed.
