The galaxy presents as a largely featureless, elliptical-like object. The core region exhibits a bright, concentrated luminosity, suggestive of a high density of stellar populations. A smooth, albeit diffuse, halo extends outwards from the central region. There's a subtle color gradient visible, with the core appearing yellower compared to the outer regions which have a slightly bluer tint. This could suggest older stellar populations are concentrated in the galaxy's center, while younger stars may populate the outskirts, though this difference is subtle. There is no definitive evidence of spiral arms, rings, or bar structures. No major disturbances or merger events are immediately apparent; the overall structure appears relatively undisturbed. The galaxy possesses a generally rounded morphology, lacking any significant elongation.
