The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a centrally concentrated light profile, with a gradual decrease in surface brightness moving outward from the core. The color appears to be dominated by redder wavelengths, suggesting an older stellar population and a relative lack of ongoing star formation. There is no discernible disk structure or spiral arm features visible. The overall shape is generally round, showing minimal signs of tidal disturbances or interactions with other galaxies. The object appears to be a massive system, based on its brightness and size at its inferred distance. There is a small chance that there is some kind of very minor disturbance, but overall it is a mostly undisturbed galaxy.