The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a bright, concentrated core region, gradually decreasing in intensity towards its outer edges. There is very little evidence of spiral arms or significant dust lanes, indicating a lack of ongoing major star formation. The morphology suggests a well-evolved system, likely dominated by older stellar populations. The galaxy presents a generally round appearance with no apparent signs of tidal disturbances or recent merger activity. The color appears to be dominated by yellow and redder wavelengths, suggesting a population of older, cooler stars. Overall, the galaxy appears to be a mature, relatively quiescent system.
