The galaxy presents a relatively smooth, elliptical morphology. It is dominated by a yellowish-orange hue, indicative of an older stellar population with a lower rate of current star formation. The galaxy appears somewhat elongated, deviating slightly from a perfectly circular shape. There is a subtle hint of a tidal disturbance or interaction, possibly suggesting a recent or ongoing merger event. The galaxy lacks well-defined spiral arms or prominent dust lanes, further supporting the classification as an elliptical galaxy. The core exhibits a concentrated brightness, while the outer regions gradually fade into the background. Overall, the galaxy appears to be a fairly massive system.
