The galaxy presents as a single, centralized object. It appears to be a galaxy with a high degree of symmetry and concentration. The light distribution suggests a relatively smooth profile, transitioning from a brighter core to a dimmer outer region. There is no clear evidence of spiral arms or a distinct disk structure, suggesting that it could be an elliptical galaxy. The overall color profile indicates a redder core transitioning to a greener surrounding aura, this implies a population of older stars. The presence of a bright, compact core suggests the potential existence of a supermassive black hole, or perhaps a central accumulation of older, redder stellar populations. The morphology appears to be undisturbed, without major tidal features, implying a relatively isolated existence.
