The galaxy presents as a roughly elliptical, centrally concentrated object. It exhibits a smooth, featureless morphology in this imaging. A subtle color gradient is observable, with the central region displaying a yellowish-orange hue, potentially indicating an older stellar population, while the outer regions appear slightly bluer, hinting at the presence of younger stars or ongoing star formation activity. The overall shape is predominantly round, lacking any distinct spiral arm structures or bar features, though a very slight disturbance or faint feature could be present near the edges. There is no strong evidence of a major merger in progress, though a minor interaction cannot be entirely ruled out.
