The galaxy appears as an elliptical or lenticular type. Its morphology is smooth and centralized, with a high degree of symmetry. There is little or no evidence of spiral arms or significant disk-like structures. The galaxy is dominated by light at the red end of the spectrum, indicating that it is composed primarily of older stars. There is no strong evidence of ongoing, active star formation, however, there could be very low levels of star formation occurring. There is only slight evidence of any disturbance or tidal features, suggesting that it has not recently experienced a major merger event. The galaxy is moderately luminous. Its shape is more in-between round and elliptical, but appears mostly round.
