The galaxy presents a predominantly elliptical morphology, exhibiting a smooth light distribution that gradually diminishes from the central core outwards. The core appears bright and slightly yellowish, possibly indicating a concentration of older stellar populations. Fainter, bluer light is observed in the outer regions of the disk, suggesting the presence of younger stars. The galaxy's shape exhibits an axial ratio consistent with a slightly flattened spheroid. There are subtle indications of possible disk features, but these are not well-defined. There are no apparent signs of major mergers or tidal disturbances.
