The galaxy presents as a relatively compact structure with a smooth, elliptical morphology. Its color appears to be largely consistent, with subtle variations suggesting a range of stellar populations. The overall form indicates a spheroid-dominated system, with minimal evidence of spiral arms or significant disk features. The galaxy's intermediate axial ratio suggests it is neither perfectly spherical nor highly flattened. There is a slight suggestion of a minor disturbance or interaction affecting its overall form. The galaxy does not appear to be undergoing a major merger event, although there is some asymmetry. Observations indicate it is a massive galaxy with ongoing, though suppressed, star formation. 
