The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. There is a slight elongation, deviating marginally from a perfectly circular shape. The galaxy exhibits a color gradient, with a central region that appears bluer, potentially indicating the presence of a younger stellar population or active star formation. The outer regions display a redder hue, possibly indicative of an older stellar population. There is faint evidence of minor tidal disturbances or interactions, though the overall structure remains largely undisturbed.
