The galaxy exhibits a moderate redshift, placing it at a considerable distance. It has a relatively large estimated size. Morphologically, it presents as predominantly smooth, although subtle features may be present. The shape is generally rounded, with a slight deviation from perfect circularity towards an intermediate form. There is weak evidence for minor disturbances, but appears to be generally isolated with no major ongoing mergers. Color indices suggest a redder population, indicating older stars and/or significant dust obscuration. The high inferred stellar mass and low specific star formation rate point towards a quiescent galaxy, possibly a massive early-type system transitioning off the blue sequence.
