The galaxy presents a morphology consistent with an elliptical or lenticular type. It exhibits a generally smooth, centralized light distribution with no obvious spiral arm structure or significant dust lanes visible. The object displays an elongated, but not extremely flattened, spheroidal shape, appearing slightly more extended than a perfectly circular distribution. The color profile appears relatively uniform across the galaxy, showing a bias toward redder wavelengths, indicative of an older stellar population and subdued star formation. There is no strong evidence of tidal features or ongoing merger activity, suggesting it is a relatively undisturbed system. The overall appearance is that of a quiescent, passively evolving galaxy with a substantial stellar mass.
