The galaxy presents a smooth, elliptical morphology. The central region exhibits a concentrated, bright core, suggesting a substantial stellar population. The overall color is predominantly yellow-red, indicative of an older stellar population with a comparatively lower rate of ongoing star formation. There is no observable spiral structure or disk component and no major disturbances due to merging. There appears to be some minor disruption in the galaxy. The galaxy appears to be generally round, but it is not perfectly spherical.
