The galaxy presents an elliptical morphology with a high degree of central concentration. The light profile appears smooth and relatively featureless, lacking prominent spiral arms or distinct dust lanes. The color is generally yellowish-white, suggesting a stellar population dominated by older, evolved stars, with potentially lower rates of on-going star formation. The galaxy appears to be somewhat elongated. There are no obvious signs of tidal disturbances or major interactions with other galaxies. The galaxy's half-light radius is relatively compact.
