The galaxy appears to be an elliptical galaxy, characterized by a generally smooth and diffuse light distribution. The central region is a bright yellowish-white, possibly indicating an older stellar population. There is a very slight elongation of the galaxy along one axis, although the overall shape remains largely spherical. Faint, diffuse light extends outwards from the core, fading gradually into the background. There are no obvious spiral arm structures, dust lanes, or signs of ongoing or recent star formation. There is a slight redder area on the bottom portion of the galaxy. Overall, the galaxy seems undisturbed with no signs of major merger events in its recent history.
