The galaxy presents as a largely featureless, elliptical or spheroidal object. It exhibits a smooth, rounded morphology, with a high degree of circular symmetry. The light distribution appears concentrated toward the center, fading gradually outward. The color profile suggests a stellar population dominated by older stars.

There is no visible evidence of spiral arms, bars, or significant dust lanes. No obvious signs of active star formation. The galaxy shows no distinct tidal features or signs of ongoing merger activity, although faint disturbances cannot be entirely ruled out.
