The galaxy presents a generally smooth morphology with a primarily elliptical shape, nearly circular, but with a slight elongation along one axis. The central region exhibits a bright concentration of light, potentially indicative of an active galactic nucleus or a dense stellar population. The light appears to be primarily red and orange with a small, less defined halo that extends outwards from the core. There is also a feature that resembles a merging event or some kind of tidal distortion to one side of the galaxy. There are also some suggestions of internal structure that may contain hints of a disk component.
