The galaxy appears to be an elliptical, with a smooth, centrally concentrated morphology. It exhibits a golden hue, possibly indicating an older stellar population. The light distribution suggests a high degree of radial symmetry, with a relatively homogenous texture lacking any distinct spiral arm structures or prominent dust lanes. The galaxy has a slightly elongated shape. There is no clear evidence of tidal disturbances or ongoing mergers; the galaxy appears relatively isolated and undisturbed. 
