The galaxy presents as a largely featureless, elliptical morphology, appearing smooth in structure. Its color profile suggests an older stellar population, exhibiting a redder hue in the central bulge region. There is a slight gradient towards bluer colors in the outer regions, indicating the possibility of some ongoing, albeit limited, star formation. The shape is somewhat elongated, leaning towards an intermediate shape, deviating slightly from a perfectly circular form. There is no strong evidence of major disturbances or merging activity from this image.
