The galaxy presents as a centrally concentrated elliptical, appearing relatively smooth in morphology, with a high degree of rotational symmetry. The radial light profile decreases gradually from the core, exhibiting a Sersic index suggestive of a de Vaucouleurs profile. The color gradient is subtle, with the central region appearing slightly yellower than the outer regions, potentially indicating an older stellar population towards the core. The isophotes are moderately elliptical, showing a minor axis to major axis ratio indicating it is not a perfect circle but deviates slightly from a perfect round shape. There is no obvious sign of spiral arms, bars, or dust lanes. No clear evidence of recent or ongoing major merger activity is apparent, although a slight asymmetry cannot be ruled out at this resolution.
