The galaxy presents as a centrally concentrated, elliptical-like structure. The core exhibits a bright, yellowish-orange hue, suggesting an older stellar population dominating the nuclear region. There is a faint extension visible, possibly a tidal tail or arm, suggesting past or ongoing interaction. The smooth appearance supports a classification toward an early-type galaxy, and is likely a massive galaxy with a high stellar mass. The galaxy appears to have a red shift, supporting that it is distant. Some low levels of star formation are likely occurring within the galaxy.
