The galaxy presents as a relatively smooth, centrally concentrated object with a slightly elongated shape. The core exhibits a yellowish-red hue, potentially indicating an older stellar population or dust obscuration. There appears to be a faint, greenish-blue halo surrounding the central bulge, suggesting the presence of younger, star-forming regions. Subtle asymmetry and minor disturbances in the outer regions indicate past or ongoing interactions, though it does not appear to be undergoing a major merger. There are no strong spiral arm features observed. The galaxy appears relatively isolated with no other bright objects nearby. The redshift implies that this is a relatively distant galaxy. Overall, it seems to be a massive galaxy with intermediate star formation activity.
