The galaxy presents a generally smooth and rounded morphology. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards the outer regions. The color profile suggests a relatively evolved stellar population, with a dominant yellowish-orange hue in the core transitioning to slightly bluer tones in the outer halo. No distinct spiral arm structures or significant dust lanes are discernible. There are no clear signs of tidal disturbances or ongoing major mergers, indicating a quiescent state. Minor irregularities at the outskirts may suggest minor interactions or past accretion events, but the overall structure appears largely undisturbed. The galaxy exhibits a moderate degree of redshift, indicating a substantial distance. Based on color indices, the galaxy has a low specific star formation rate, suggesting that star formation is largely suppressed.
