This galaxy presents as a relatively smooth, elliptical object. The central region exhibits a high degree of luminosity with a noticeable yellow-white hue, suggesting a population of older stars. The light intensity gradually decreases moving outward from the core. There is little indication of spiral arm structure or significant dust lanes. The overall shape is generally round, without any obvious distortions indicative of a recent major merger event. There are hints of bluer light in the fainter outer regions, suggesting some ongoing star formation, however this is subdued relative to the central bulge. There is no obvious nucleus, meaning this is likely not an active galaxy. Overall, the morphology suggests an evolved system where the majority of star formation has ceased.
