The galaxy appears as a moderately bright, flattened spheroid with a subtle but discernible asymmetry. There's a hint of tidal disturbance or interaction evidenced by a faint extension on one side, possibly indicating a recent or ongoing merger event. The galaxy's color profile suggests a relatively evolved stellar population, leaning towards redder hues. The light distribution is centrally concentrated. There is no obvious presence of spiral arms or dust lanes, so it is most likely an elliptical galaxy.
