The galaxy presents a generally smooth morphology, lacking prominent spiral arms or a well-defined disk structure. The light is concentrated in the central region, indicating a possible spheroidal or elliptical shape. The color appears to be yellowish-orange, suggesting an older stellar population with a low rate of star formation. The galaxy seems relatively undisturbed, with no obvious signs of recent mergers or major interactions. Its overall appearance suggests that it may be a massive galaxy that has largely exhausted its supply of gas for star formation.
