The galaxy presents as a somewhat elliptical, diffuse object. Its core exhibits a concentrated, bright, yellowish-white luminosity, indicating a population of older stars. The outer regions show a gradual fading in intensity. Faint blue-ish tinges are visible in these dimmer regions, possibly indicating recent star formation. Some irregularities in the outer structure are visible, hinting at minor disturbances or tidal interactions, though these are not pronounced enough to suggest a major ongoing merger. The galaxy appears generally smooth and featureless, although some elongated components are visible.
