This galaxy presents as a centrally concentrated object with a smooth, largely featureless morphology, suggesting a relatively old stellar population. It is characterized by an overall elliptical shape and a bright core, indicative of a possible supermassive black hole. A slight asymmetry is visible, possibly due to minor tidal interactions or internal dynamics, though the galaxy appears primarily relaxed. Color gradients show a redder hue at the core, likely representing older, cooler stars, with a bluer periphery suggesting some ongoing, albeit low, levels of star formation in its outer regions. There is no obvious evidence of spiral arms or significant dust lanes.
