The galaxy appears to be a relatively smooth, elliptical galaxy with a bright central bulge. It exhibits a yellowish core, suggesting an older stellar population dominates the central region. Surrounding the core is a more diffuse, bluish halo or envelope. This halo might indicate the presence of younger stars or possibly ongoing, albeit subdued, star formation at the galaxy's periphery. The galaxy shows an overall elliptical shape, appearing more rounded than cigar-shaped. There are no obvious signs of spiral arms or major disturbances indicative of an ongoing merger. Faint hints of features or irregularities within the halo might suggest minor gravitational interactions or past merger events, though these features are subtle and don't dominate the overall morphology.
