The galaxy presents an overall morphology that appears to be moderately disturbed with potentially a few minor features disrupting its overall shape. The light distribution exhibits a relatively smooth central concentration, with a subtle elongation suggesting a departure from perfect sphericity. There is a region of distinct color variation, where the light is more yellow, hinting at possible variations in stellar populations or dust content within that area. The general shape is neither perfectly round nor markedly elongated, residing somewhere in between these extremes. The features are suggestive of an ongoing interaction or internal dynamic process. Overall, the galaxy displays characteristics that point towards a system that is not completely settled or quiescent.
