The galaxy appears to be a relatively smooth, elliptical-type galaxy with a centrally concentrated bulge. Its light is dominated by older stellar populations, as evidenced by the reddish-yellow hue in the outer regions. A subtle color gradient is observed, with the central region exhibiting a slightly bluer tint, potentially indicating a small population of younger stars or ongoing low-level star formation in the core. The galaxy shows a high degree of circularity. There is no obvious evidence of spiral arms, a bar, or any significant tidal disturbances or interactions with neighboring galaxies in this image. The overall structure suggests a quiescent galaxy with a modest stellar mass.
