The galaxy presents as a fairly smooth object with a concentrated central bulge. The light distribution suggests an elliptical morphology, with a high degree of central concentration. The overall color appears to be a yellowish-red hue, indicating an older stellar population with a relatively low rate of on-going star formation. There appears to be a slight tidal disturbance, though it is very minor. The galaxy does not appear to be actively merging. The observed properties are consistent with an early-type galaxy at a moderate cosmological distance.
