The galaxy exhibits a moderate redshift, indicating a significant distance. It appears elliptical or lenticular, with a generally smooth morphology and minimal discernible substructure. The galaxy is elongated, but not strongly so. There may be some indication of tidal features, suggesting that it may be undergoing or have recently undergone a merger event with another galaxy. There is no apparent evidence of a prominent disk or spiral arms. The galaxy exhibits an orange/yellow hue, indicating that it likely contains an older stellar population. The galaxy's star formation rate appears to be relatively low.
