The galaxy appears to be an elliptical galaxy with a smooth, featureless morphology. It exhibits a concentrated central bulge that diminishes outwards. The galaxy's light profile suggests an older stellar population, with a color index leaning towards redder wavelengths, indicating lower levels of ongoing star formation. However, there may be minimal star formation occurring, or perhaps a past merger event. It appears undisturbed, with no prominent tidal features or asymmetries suggesting a recent major merger event. However there could be a minor disturbance, or a merger event, evidenced by a slight irregularity in its overall shape. It has intermediate roundness, and the shape is not perfectly circular, leaning slightly toward a prolate shape.
