The galaxy presents as a single, dominant spheroidal component. Its overall form appears smooth and elliptical, with high degree of central concentration. The light is yellowish-red, suggesting a population of older stars. A faint, slightly elongated structure is observed to the left of the main body, potentially indicative of a minor tidal disturbance or interaction with a smaller companion galaxy. The smooth morphology suggests a well-mixed stellar population, consistent with an early-type galaxy classification.
