The galaxy presents as a relatively smooth, elliptical morphology. Its light profile appears centrally concentrated, with a gradual decrease in intensity outwards. The color is generally yellowish, suggesting a population of older stars with lower rates of on-going star formation. There are no obvious spiral arm structures, bars, or significant dust lanes visible in the image. The overall appearance indicates a system that is likely well evolved. It does not appear to be undergoing any major mergers or tidal disturbances, maintaining a settled structure.
