The galaxy presents as a somewhat elliptical object, elongated along its major axis. It exhibits a smooth, diffuse light profile with a concentrated central bulge that appears yellowish-white in color, suggesting an older stellar population. The outer regions of the galaxy are fainter and display a slight blue tinge, which could indicate the presence of younger, hotter stars, or possibly ongoing, low-level star formation. No distinct spiral arm structures or dust lanes are readily apparent. The galaxy appears relatively isolated, showing no obvious signs of tidal interaction or recent merger events. Its overall morphology suggests a galaxy that is undergoing a relatively quiescent phase of stellar evolution.
