The galaxy appears to be an elliptical type, displaying a generally smooth and concentrated light distribution. It exhibits a high degree of central concentration. The overall shape is predominantly round with only slight deviations. There is no apparent disk structure or spiral arm morphology visible. Minimal signs of ongoing or recent merger activity are present, with no prominent tidal tails or distortions. The galaxy has a calculated redshift, indicating it is at a considerable distance. Its absolute magnitude is relatively bright. The estimated stellar mass is substantial, indicating it's a massive galaxy. The star formation rate is relatively low, suggesting it is a quiescent galaxy with an older stellar population. The specific star formation rate is also low.
