The galaxy appears as a concentrated, elliptical-like structure with a smooth, luminous profile. The central region exhibits a pronounced brightness, suggesting a substantial concentration of stars. The color gradient transitions from a yellow-gold core to a slightly greener hue in the outer regions, which may indicate some ongoing, although diminished, star formation activity. There is no clear evidence of spiral arms or a distinct disk structure. The galaxy's morphology suggests it is a relatively evolved system, likely a massive galaxy with a high stellar mass and low specific star formation rate. There are no obvious signs of a recent or ongoing major merger, although minor disturbances or interactions cannot be ruled out based on the image alone.
