The galaxy presents as a smooth, elliptical form. Its shape is not perfectly round but exhibits a moderate elongation. The light distribution appears to be concentrated towards the center, with a gradual fading towards the outer edges. The dominant color is a yellowish-orange hue, potentially indicating an older stellar population and/or dust obscuration within the galaxy. There is a subtle hint of bluish color on the edges of the galaxy, which may be indicative of younger stars. There are no obvious spiral arms or distinct features to suggest ongoing major merging activity, although there might be some minor disturbances in its morphology.
