The galaxy appears as a single, relatively smooth concentration of light. There is a hint of a more intensely luminous core region. The overall color profile is slightly redder, which suggests a population of older stars dominating the light output. Based on the shape, it seems to be more circular than elongated. There is no clear indication of spiral arms or a well-defined disk structure from this image. No major signs of active galactic nuclei are obviously visible, and there are no major disturbances detected. The smooth appearance is suggestive of a galaxy undergoing minimal star formation.
