The galaxy presents as a relatively smooth, elliptical structure. The color profile is dominated by redder hues with a small portion of the light being green and a bit less being blue, suggesting a population of older stars and a low ongoing star formation rate. The galaxy appears well-defined, with a high degree of radial symmetry. There is no obvious evidence of spiral arms or a prominent disk. No signs of recent or ongoing major merger activity can be observed. The overall morphology suggests an evolved system with a dominant spheroidal component.
