The galaxy presents as a moderately luminous object with a smooth, concentrated morphology. The overall shape is somewhat elliptical, appearing more elongated than perfectly circular. The color profile suggests an older stellar population, with a dominant yellowish hue that may indicate a lack of significant ongoing star formation. Some disturbances may be present as minor asymmetries are visible in the outer regions of the galaxy. No prominent spiral arms or distinct features, such as bright knots of star formation, are clearly discernible. 
