The galaxy exhibits a flattened, disk-like morphology when viewed from our perspective. The central bulge appears yellowish-white, possibly indicating a population of older stars. Surrounding the bulge is a prominent ring-like structure showing a red hue, hinting at ongoing star formation, dust or a population of stars different from those in the central bulge. Faint blue coloring can be observed within the ring, perhaps suggesting the presence of younger, hotter stars. A very faint greenish glow can be observed directly behind the ring. The overall smoothness of the galaxy suggests that it is relatively undisturbed. There are hints of minor asymmetry, indicating the possibility of interactions with smaller galaxies or gravitational disturbances. There may be a tidal tail stretching from the top of the galaxy.
