The galaxy presents a largely smooth, elliptical morphology with a concentrated central bulge. The light distribution is dominated by a yellow-orange hue, suggesting a population of older stars. There is a slight flattening, but the galaxy appears mostly round. Hints of a faint, diffuse disk are visible surrounding the central bulge, although distinct spiral arms are absent. There is a subtle color gradient, with the central region appearing more yellow than the outer regions. No obvious signs of recent major merger activity are visible.
