The galaxy presents as a centrally concentrated, elliptical structure. Its overall form appears smooth, with no immediately obvious spiral arms or significant dust lanes. The central bulge is luminous and dense, fading outwards towards the edges. The object's color is predominantly bluish-white near the core, indicating a likely presence of younger, hotter stars in the bulge. The outer regions exhibit a gradual shift towards redder hues, which would suggest an older stellar population. Its shape appears somewhat elongated rather than perfectly spherical. There is a very slight hint of asymmetry, possibly due to a minor gravitational interaction. The galaxy does not show any dramatic signs of an ongoing merger, but this subtle irregularity warrants further inspection.
