This galaxy presents as a smooth, centrally concentrated object. The light distribution is fairly symmetrical, lacking any obvious spiral arms or a distinct disk-like structure. There is a slight elongation visible, but the overall shape is closer to round than a highly elongated or cigar shape.

The galaxy's color appears primarily white, with some subtle variations in the blue end of the spectrum at the edges of the object. This suggests the presence of a population of young stars that are actively producing hot gas. The smoothness in the image suggests that the galaxy is either an elliptical or lenticular type.

The lack of major disturbances or merger features indicates a relatively stable and undisturbed morphology. Close inspection reveals no indication of a recent or ongoing major merger event.