The galaxy presents as a slightly elongated elliptical or lenticular structure, displaying a relatively smooth morphology with no prominent spiral arms or distinct features discernible at this resolution. The central region exhibits a concentrated luminosity gradient, suggesting a dense galactic nucleus or bulge. There is a color gradient visible, with a more yellow-red hue in the center becoming more green towards the outer regions of the main disk. A subtle suggestion of some disk morphology is present, but it is not a strong indication of a spiral structure. Based on the undisturbed morphology and light distribution, there is no obvious indication of a major ongoing merger event. The overall appearance suggests a relatively quiescent galaxy.