The galaxy presents a smooth, centrally concentrated morphology. Its shape is neither perfectly round nor highly elongated, appearing somewhat elliptical. There is a subtle suggestion of a disk structure, though it is not sharply defined, as it contains a bright central bulge. There is no indication of strong tidal features, major disturbances, or an ongoing merger. The light is dominated by a blue hue, more prominent towards the center. This might indicate a population of younger, hotter stars concentrated toward the galaxy's core.
