The galaxy presents a smooth, elliptical morphology with a high degree of central concentration. Its light profile suggests a relatively old stellar population, with a dominant yellowish hue in the core. There are no visible spiral arms or dust lanes indicative of ongoing star formation. The galaxy appears well-isolated, showing no obvious signs of recent or ongoing merger activity. It is moderately luminous, suggesting a considerable stellar mass. The overall shape indicates a likely spheroid-dominated system, possibly of type E3-E5 on the Hubble sequence.
