The galaxy presents as a primarily smooth, elliptical structure with a concentrated central bulge. The dominant color is a yellowish-orange hue, suggesting a population of older stars with relatively low ongoing star formation. The shape appears nearly circular, exhibiting minimal signs of distortion or tidal features indicating recent or ongoing interactions with other galaxies. No distinct spiral arms or prominent dust lanes are discernible. There is a slight gradient in color intensity from the central bulge outwards, becoming fainter at the edges. The overall morphology suggests a galaxy that is evolved and stable, with a high degree of symmetry.
