The galaxy appears as a slightly elongated, diffuse object with a generally smooth morphology. It exhibits a color gradient, appearing bluer toward its outer regions and redder towards the central core, potentially indicating differing stellar populations. The main body of the galaxy has an intermediate roundness, neither perfectly spherical nor highly elongated. There are subtle disturbances present within the galaxy's structure, which could be due to a minor interaction or internal processes. Although, the galaxy overall appears relatively isolated with no major merging events evidently taking place. The approximate size of the galaxy is around 6 kiloparsecs.
