The galaxy appears as a relatively bright, elliptical object. It exhibits a high degree of central concentration, with a luminous core gradually fading into a more diffuse halo. The galaxy's color is generally yellowish-white, which suggests a population of older stars. There is little evidence of spiral arm structure or significant dust lanes. The overall shape indicates a likely classification as an elliptical galaxy, with a smooth, round appearance. There is no strong visual evidence of any major ongoing merger activity or significant tidal disturbances; the shape seems relatively undisturbed.
