The galaxy presents an elliptical morphology, appearing elongated with a high degree of axial ratio. Its overall color profile suggests a redder, more evolved stellar population, with the concentration of light indicating a centrally dominant bulge. There is no clear evidence of spiral arm structures or significant dust lanes visible within the image, although minor irregularities at the edges could suggest some tidal disturbance or recent interaction. The smoothness of the light distribution implies a well-mixed stellar population.
