The galaxy appears to be a relatively smooth, elliptical galaxy. The central region exhibits a high concentration of light, suggesting a dense core. The light distribution gradually decreases toward the outer edges, with no distinct spiral arm structures visible. There is some suggestion of faint and diffuse outer regions, but the overall morphology indicates a relatively relaxed and undisturbed system. The color is generally redder than blue, which would indicate that the galaxy is mainly composed of older stars. The general lack of prominent features or tidal tails suggests that it has not undergone a major merger in the recent past. The overall roundness and lack of significant disturbances are consistent with an evolved elliptical galaxy.
