The galaxy presents as a largely amorphous structure. It exhibits a somewhat elliptical morphology, appearing more rounded than elongated. The light distribution appears relatively smooth and centrally concentrated, with a gradual decrease in intensity from the center outwards. There is little indication of spiral arms or distinct features. The color profile suggests a dominant population of older stars, displaying a yellowish hue. There is a faint indication of some blue, implying there may be some younger star formations. There is no sign of any other galaxy interaction.
