This appears to be a spiral galaxy with a prominent, bright central bulge. The bulge is slightly elongated. The galaxy displays a well-defined disk structure. I observe what appear to be spiral arms originating from the central bulge, though they are tightly wound and somewhat difficult to discern clearly. These arms seem to host regions of star formation. Overall, this galaxy appears relatively undisturbed. The galaxy is not seen edge on, so the spiral arm structure is still somewhat visible. The color gradient suggests the bulge is composed of older stars, while the disk contains populations of both young, bright stars and older stars. There is evidence of a bar like structure through the bulge, adding complexity to the morphology. The disk tapers off gradually into the surrounding space.
