The galaxy presents as an elliptical or lenticular type system. It is relatively compact, with a concentrated central region showing a smooth, mostly featureless morphology. The light distribution suggests a centrally dominant spheroid component. A moderate level of on-going star formation is indicated by a slightly bluish hue in the outer regions, though its contribution is small. There is some evidence of disturbance in the galaxy's structure, suggesting a possible past or on-going interaction or merger event. This is indicated by some asymmetries in the outer isophotes.
