The galaxy appears to be a relatively small, well-defined elliptical galaxy. It exhibits a smooth, featureless morphology with a high degree of central concentration, gradually fading towards its periphery. The light distribution suggests a mostly homogenous stellar population. The galaxy presents a slight elongation in its shape, deviating somewhat from a perfect spherical form. No significant signs of ongoing merger activity or tidal disturbances are apparent, though a minor disturbance cannot be ruled out due to the resolution. Its color is a slightly blue-ish white, which may indicate some active star formation, though it is likely low.
