The galaxy appears to be a relatively smooth, rounded system, exhibiting a concentrated central bulge that is bright and slightly yellow in color, indicating an older stellar population. The outer regions of the galaxy appear more diffuse. There is a lack of any clear spiral arm structure or significant dust lanes, which suggests this may be an elliptical galaxy or a lenticular galaxy. It is difficult to discern any fine details within the galaxy given the limitations of the image resolution, such as star clusters or areas of active star formation. There are no obvious signs of a major ongoing merger or tidal disturbances, though minor interactions cannot be ruled out completely. The round shape of the galaxy suggests that it is viewed close to face-on.
