The galaxy presents as a relatively smooth, elliptical-like morphology. The central region exhibits a bright, concentrated core that gradually diffuses into the outer regions. There is a lack of distinct spiral arm structures or prominent dust lanes visible. The galaxy appears more rounded in shape, with a slight elongation noticeable. Color gradients suggest a stellar population that is predominantly older, with a yellowish hue in the central regions, potentially indicating a higher concentration of evolved stars. There is faint blue light in the outer regions, showing some amount of ongoing star formation, albeit at a lower rate compared to typical spiral galaxies. The overall structure shows no signs of major disturbances or ongoing merging activity.
