The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a roughly elliptical morphology, appearing neither perfectly circular nor highly elongated. There is a central, bright core that is yellow in color. The light smoothly dissipates from the core outwards, with a redder halo and hints of a blue outer region. There is no clear evidence of spiral arm structure or a prominent disk within the limitations of this image resolution, and no obvious signs of recent or ongoing major mergers are present. The light distribution indicates a relatively evolved system, potentially an elliptical galaxy. The color profile suggests a population of older stars in the core, with some evidence for younger, bluer stars on the outer edges of the galaxy. Minor disturbances cannot be ruled out given the resolution.
