The galaxy presents a generally smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, with the intensity decreasing gradually outwards from the core. The core region displays a subtle yellowish hue, possibly indicative of an older stellar population dominating in this area. The outer regions show a fainter, slightly bluer color, suggesting the presence of younger stars. There is no clear evidence of spiral arms or a well-defined disk structure. The overall shape is relatively round, with a slight elongation. There are no obvious signs of major mergers or strong tidal disturbances, though some minor irregularities in the outer halo cannot be ruled out. The galaxy's light distribution suggests it is a relatively massive system, with ongoing, but not exceptionally vigorous, star formation.
