The galaxy exhibits an elliptical morphology, appearing as a diffuse, elongated structure. Its overall color suggests a mix of stellar populations, with a slightly reddish hue indicating the presence of older stars. The galaxy displays a smooth profile, lacking any distinct spiral arms or prominent dust lanes. The light is concentrated towards the center, gradually fading toward the outer edges. The shape indicates a significant amount of inclination. There is no obvious indication of recent or ongoing major merger activity.
