The galaxy presents as a relatively smooth, centrally concentrated object with a slightly elongated morphology. The light distribution suggests a largely spheroidal structure, potentially an elliptical galaxy or a lenticular galaxy viewed at an oblique angle. There is a subtle color gradient, with a slightly bluer hue in the central region, possibly indicating a small amount of ongoing star formation. No distinct spiral arms or prominent dust lanes are visible. A slight asymmetry might suggest a minor gravitational interaction or past merger event.
