The galaxy appears as a moderately bright, elliptical-shaped object. Its central region exhibits a high degree of smoothness, with a gradual decrease in luminosity towards the outer edges. There is no evidence of strong spiral arm structures, and it seems that any disk components it may have are weak. The color profile appears relatively uniform across the galaxy, suggesting an older stellar population. The galaxy's elongated shape indicates a possible deviation from a perfect spherical structure, and the possibility of it being a spiral galaxy viewed at a high inclination. There is no obvious sign of major mergers or tidal disturbances; however, a very slight asymmetry cannot be ruled out.
