The galaxy appears as a fairly smooth, centrally concentrated object with an elliptical morphology. Its color profile suggests an older stellar population dominating the light output, with a notable absence of strong blue emission indicative of recent star formation. The galaxy exhibits a slight elongation, not quite spherical but also not highly flattened. There's no immediately apparent evidence of major tidal disturbances or ongoing mergers. Subtle irregularities in the light distribution might indicate minor disturbances or internal structures, but overall the galaxy presents a relatively quiescent and evolved appearance.
