The galaxy presents an elliptical morphology, appearing generally smooth and centralized, with a high degree of central concentration, and a faint stellar halo. The light profile suggests it is mostly featureless, lacking prominent spiral arms or a discernible bar. The galaxy exhibits a slight color gradient with a yellower central region, possibly indicating an older stellar population within the bulge, transitioning to slightly bluer hues towards the outskirts, which may suggest the presence of younger stars or some ongoing star formation in the outer regions, but the star formation rate is slow. There is no distinct evidence of ongoing major mergers. It is of considerable size.
