The galaxy presents a primarily smooth morphology, with a round appearance. It exhibits a concentrated central bulge, which appears to be older stellar populations, indicating a higher concentration of evolved stars. There is evidence of a weak disk or arm-like feature, although these features do not dominate the overall structure. The galaxy appears relatively isolated. There is a red-shifted color, indicating that the galaxy is at a significant cosmological distance. Based on the color indices, the galaxy is likely actively forming stars, although the exact rate is uncertain. Overall, the galaxy is likely a massive galaxy with a substantial stellar mass.
