The galaxy presents a generally smooth and rounded morphology. There is no indication of prominent spiral arms or a well-defined disk structure. The galaxy appears to be relatively compact, with a centrally concentrated light profile that diminishes outwards, creating a somewhat fuzzy edge. The light emanating is mostly in the yellow and orange wavelengths, with a slight green hue. The galaxy appears to be isolated, without any clear signs of ongoing major merger activity or significant tidal disturbances. Close inspection does not reveal any significant fine structure, and the overall impression is that of a mature system.
