The galaxy presents a relatively smooth, elliptical morphology, with a noticeable central bulge that appears quite luminous. The light distribution is concentrated toward the center, indicative of a high stellar density in the core. The galaxy exhibits a generally regular structure, lacking prominent spiral arms or obvious signs of major disturbances. Its overall color suggests a population of older stars, with a discernible redder hue, and there seems to be a relatively low level of current star formation. The shape leans towards being somewhat elliptical, though it is not perfectly spherical. There's a very minor indication of a slight tidal disturbance in the form of a faint extension or asymmetry. The galaxy appears as a single, relatively well-defined object, without any clear signs of being actively involved in a major merger event.
