The galaxy appears to be a relatively smooth, elliptical-like structure. It has a concentrated central bulge that emits a strong yellowish light, potentially indicating an older stellar population. Moving outwards, there's a slight fading in brightness and a shift towards a redder hue, which may suggest a declining density of stars or the presence of dust absorption within the galaxy's outer regions. The overall shape seems somewhat elongated, lacking distinct spiral arm structures. There isn't any obvious indication of tidal disturbances or major ongoing merger events. It is likely a well-established, evolved galaxy.
