The galaxy presents as a moderately bright, elliptical object with a smooth, diffused light profile. The core exhibits a yellowish hue, suggesting an older stellar population. Moving outwards from the center, the galaxy displays a slight bluing in the outer regions, possibly indicating the presence of younger, hotter stars or recent star formation. The shape is somewhat elongated, deviating slightly from a perfectly circular form. There is no apparent dust lane or spiral arm structure visible. The galaxy shows no obvious signs of major disturbances or mergers.
