The galaxy presents as a fairly well-defined elliptical object with an apparent smooth morphology. A bright central bulge is visible, exhibiting a yellowish hue suggesting an older stellar population and reduced recent star formation. The galaxy’s outer regions show a faint, diffuse halo extending outwards, transitioning to a bluer color, potentially indicating the presence of younger, hotter stars or ongoing, albeit limited, star formation activity within the disk. While the main body of the galaxy appears relatively undisturbed, a slight asymmetry or subtle extension on one side may suggest a minor gravitational interaction or possible past merger event. There is no obvious dust lane or spiral arm structure visible in the image. The galaxy exhibits a generally regular elliptical shape.
