The galaxy presents as a centrally concentrated object with a smooth, relatively featureless morphology. The overall shape appears elliptical, with a slight elongation. The color profile suggests a dominant population of older stars, exhibiting a yellowish-red hue throughout the main body. There is a brighter, more intense core region, possibly indicating a higher concentration of stars and/or a central supermassive black hole. Evidence of spiral arms or significant dust lanes is absent. Subtle color variations within the galaxy's outer regions hint at varying stellar populations or potential low-level star formation activity. However, the overwhelming impression is that of a quiescent, evolved system. Any signs of ongoing or recent merger events appear minimal, with a largely undisturbed structure.
