The galaxy presents an elliptical morphology, appearing more elongated than perfectly spherical. The light distribution is concentrated towards the center, indicating a prominent galactic nucleus. A significant fraction of the galaxy's light appears smooth and relatively featureless. There seems to be a minor irregularity or possible disturbance in its overall structure, but no signs of a major merger. The color profile suggests the presence of a moderately evolved stellar population, with a mix of older stars. The galaxy seems to have a moderate star formation rate.
