The galaxy presents a generally smooth and centrally concentrated light profile. The shape appears largely elliptical, tending towards an in-between roundness, with only a slight elongation. There is an apparent color gradient, with a more yellow/red core transitioning to slightly bluer hues in the outer regions, suggesting potentially older stellar populations concentrated in the center with pockets of younger stars in the more distal regions. No distinct spiral arm structures or prominent dust lanes are discernible, indicating a featureless, or smooth morphology. There is no obvious indication of any major merger events currently taking place, or any significant tidal disturbances.
