The galaxy appears as a relatively smooth, centrally concentrated object. It exhibits a morphology consistent with an elliptical galaxy or a lenticular galaxy viewed face-on. The color profile suggests a population of older stars, with a dominant yellowish-orange hue in the central regions, possibly indicating a lack of significant ongoing star formation. There may be some very low level ongoing star formation in the outer regions. The galaxy shows no obvious signs of spiral arms or a prominent disk structure, nor does it show any signs of major disturbances or interactions with other galaxies. It exhibits a high degree of roundness. There is some color variation from the center to its outer regions.
