The galaxy appears as a flattened, elliptical structure. The central region is a bright, concentrated bulge, exhibiting a yellowish-orange hue. This suggests a population of older, cooler stars. Fainter, bluer light extends outwards from the central bulge in a disk-like structure. This implies the presence of younger stars and possibly ongoing star formation in these regions. There is some irregularity to the outer disk, with hints of faint spiral arms. Overall, the galaxy displays characteristics of both elliptical and spiral galaxies. It is neither a purely smooth elliptical nor a fully developed spiral, suggesting a galaxy of intermediate morphology.
