The galaxy presents as a somewhat elongated, elliptical structure with a smooth, diffuse appearance. A bright central bulge is visible, transitioning gradually outwards to a fainter, less defined halo. The color profile suggests an older stellar population, with a dominant yellowish-orange hue throughout the galaxy. There is little evidence of spiral arms or distinct dust lanes. Based on the galaxy's morphology, it appears to be relatively undisturbed, without significant signs of ongoing or recent merger activity.
