The galaxy presents as a centrally concentrated object with a generally smooth appearance. It exhibits a roughly elliptical morphology with a dominant, bright central bulge or core. The light appears relatively uniform, suggesting a lack of distinct spiral arms or significant dust lanes. There's a subtle color gradient observable, transitioning from a slightly bluer hue in the central region to a somewhat redder color towards the outer edges. Based on these characteristics, the galaxy is most likely an elliptical galaxy. The relatively high central concentration suggests an older stellar population.
