The galaxy presents as a somewhat elongated, lenticular-like structure. It appears relatively smooth and featureless, lacking prominent spiral arms or a distinct central bulge when compared to a spiral galaxy. The color profile suggests a population of older stars, with a bias towards redder hues. There is a subtle gradient in brightness from the center outwards, indicating a concentration of stellar mass in the core region. No obvious signs of recent major merger events are apparent. There is no clear indication of active star formation regions.
