The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge that radiates brightly, indicating a high stellar density in the core. The color of the central region appears yellowish-white. Moving outward from the core, the luminosity diminishes, transitioning into a fainter, more diffuse halo. There appears to be a slightly flattened shape rather than a perfect sphere. There are no distinct spiral arm structures visible. No significant dust lanes or prominent star-forming regions are discernible from the image. The outer edges fade gradually into the background, indicating a lack of a sharp boundary. The general appearance suggests an older stellar population, with a low rate of current star formation activity. There is no visual evidence of any major ongoing merger events or strong tidal disturbances.
