The galaxy presents as a somewhat elongated, disk-like structure. The central bulge appears prominent and exhibits a yellowish-orange hue, suggesting a population of older, cooler stars. The overall smoothness of the galaxy indicates it is likely an early-type spiral or lenticular galaxy. The disk itself shows a subtle bluer tint compared to the bulge, hinting at the presence of younger, hotter stars and some ongoing star formation, although likely at a modest rate. There is a slight asymmetry to the outer edges of the disk, perhaps due to minor gravitational interactions or internal dynamical processes. No distinct spiral arm structure or prominent dust lanes are discernible in this image.
