The galaxy presents as a relatively smooth, elliptical form. The central region exhibits a high concentration of light, suggesting a prominent nucleus or bulge. The light distribution appears mostly uniform, with a gradual fading in intensity towards the outer edges. There is minimal evidence of distinct spiral arms or a well-defined disk structure. The galaxy's overall color is a yellowish-white, potentially indicating an older stellar population with fewer young, blue stars. There is a slight hint of blueish color in the surrounding areas of the galaxy. No significant tidal tails, dust lanes, or other signs of recent major mergers are readily apparent. A small fraction of the galaxy's classification suggests it may be considered disk-like. The galaxy appears relatively undisturbed and quiescent.
