The galaxy presents as a luminous, elliptical form. A concentrated, yellowish-white core region dominates the galaxy's structure. The core exhibits a high degree of sphericity and luminosity, suggesting a significant concentration of stars, potentially older stellar populations. Surrounding the core, a more diffuse, bluish halo is present, extending outwards. The blue hue suggests the presence of younger, hotter stars, possibly indicating ongoing or recent star formation within the outer regions of the galaxy. The overall smooth appearance with a high degree of central concentration implies the galaxy is relatively evolved. There is no obvious spiral structure or significant dust lanes. Faint hints of possible minor tidal disturbances are suggested by the slight asymmetry in the outer halo, although a merger seems unlikely based on the overall regular form. The galaxy appears to be a massive system.
