The galaxy appears as a slightly elongated, luminous structure. Its central region exhibits a concentrated glow, suggesting a higher density of stars. The light gradually diffuses outwards from the core, transitioning into a fainter, less defined halo.

There is a hint of a disk structure with a slight angle, but the relatively smooth appearance with minimal discernible features indicates a notable absence of strong spiral arms or dust lanes. The galaxy displays a generally smooth and undisturbed morphology. The overall color suggests a mix of stellar populations, with a slightly redder central region that is indicative of older stars and a bluer disk that is indicative of younger stars.
