The galaxy presents a moderately elongated, elliptical morphology. It appears relatively smooth in structure, lacking prominent spiral arms or significant dust lanes. The central region exhibits a brighter concentration of light, suggestive of a galactic bulge. The galaxy displays a subtle color gradient, transitioning from a slightly bluer hue in the outer regions to a more yellowish-white towards the core. This color variation may indicate differing stellar populations, with younger, bluer stars populating the outskirts and older, redder stars concentrated in the center. There is a possibility of minor disturbances in the galaxy's structure, evidenced by some asymmetry, although this could also be attributed to image resolution limitations.
