The galaxy presents a largely smooth and featureless morphology, suggestive of an elliptical or lenticular type. Its shape is broadly elliptical, appearing slightly elongated rather than perfectly spherical. A central bulge is prominent, exhibiting a concentration of light. There are no obvious spiral arms or dust lanes visible. The galaxy displays a color gradient, transitioning from a yellowish core to a redder periphery. This suggests a stellar population that is older and less actively star-forming in the outer regions. There are no signs of any major mergers or tidal disturbances. The overall appearance indicates a relatively evolved galaxy with a potentially low star formation rate.
