The galaxy appears as a single, somewhat diffuse object. Its morphology suggests a system dominated by a smooth, spheroidal component. It exhibits a centrally concentrated light profile, fading gradually towards its edges. There is some color variation across the galaxy. The center of the galaxy appears to be slightly bluer, potentially indicating the presence of younger stars or ongoing star formation activity in the core. The outer regions seem redder, possibly due to older stellar populations. There is a slight distortion of the galaxy's shape, which may indicate a minor interaction or disturbance. There may be an early merger in progress.
