The galaxy appears as a centrally concentrated, smooth elliptical galaxy. It exhibits a notable color gradient, transitioning from a yellowish-white core to a bluer outer halo. The galaxy appears relatively isolated with no major merger events apparent, though there might be some minor disturbances visible in the outer regions suggesting a past interaction. The central bulge is prominent and elongated, and its light appears to dominate the overall luminosity profile. There are no distinct spiral arms or prominent dust lanes visible within the galaxy's structure. The overall shape suggests a classification towards the elliptical end of the Hubble sequence.
