The galaxy presents as a relatively smooth, elliptical-like structure, exhibiting a centrally concentrated luminosity profile. The core region appears to be comprised of older stellar populations, indicated by its yellowish-white hue. Moving outwards from the core, a subtle transition to a bluer color is observed, suggesting the presence of younger stars in the outer regions. There is a possible faint, diffuse disk-like structure. The galaxy displays a high degree of rotational symmetry, with no obvious signs of strong tidal interactions or major disturbances. Overall, the galaxy appears to be a quiescent system, likely undergoing relatively low rates of star formation.
