The galaxy presents an elliptical morphology, exhibiting a smooth and largely featureless structure. Its shape is moderately elongated. The color gradient suggests a concentration of older stellar populations in the central region, appearing yellow-white. The outer regions are less defined and exhibit bluer hues, possibly indicating ongoing, but low, star formation. There is no obvious evidence of spiral arms or a prominent disk. No significant tidal disturbances or signs of recent merging activity are apparent.
