The galaxy appears as a relatively faint, elongated structure. Its core exhibits a bright, concentrated luminosity, fading gradually outward. The morphology indicates a dominant spheroid component. The galaxy's overall color is somewhat muted, with subtle variations across its body suggesting differing stellar populations or dust distribution. There are no prominent spiral arms visible; rather, the light distribution is smoother and more amorphous. The shape is elliptical. There is evidence of minor disturbances; the overall profile does not present a completely smooth appearance.