The galaxy presents as a centrally concentrated object with a generally smooth morphology. It exhibits a roughly circular shape with a slight suggestion of elongation. The color appears yellowish-white, indicating a potential mix of stellar populations, including older, redder stars, with a possible contribution from younger, bluer stars. There's no visible evidence of distinct spiral arms, bars, or significant dust lanes. The galaxy's light profile seems to decrease steadily from the center outwards, suggesting a lack of ongoing major star formation throughout the galaxy. There is a potential minor disturbance in its morphological shape, however, the galaxy generally appears relaxed, not showing any signs of a recent or ongoing major merger event.
