The galaxy presents as a single, concentrated light source. It exhibits a smooth, elliptical morphology, suggesting a classification towards the early-type end of the Hubble sequence. There are no discernible spiral arms or a prominent disk structure. The light profile is centrally concentrated, indicative of a substantial bulge component. Color gradients appear minimal, with a generally yellowish-white hue. There is no strong evidence of ongoing major mergers or significant tidal disturbances. Minor asymmetrical features could indicate minor merger events or interactions, though the data suggests it is unlikely. The apparent circularity indicates a nearly face-on orientation relative to the observer.
