The galaxy presents a morphology somewhere between smooth and featured. A notable central bulge dominates the galaxy's luminosity, appearing largely spheroidal and displaying a yellow-white hue, indicating an older stellar population. Extending outwards from the central bulge are fainter, bluer regions indicating more recent star formation. These regions lack well-defined spiral arms. The overall shape is somewhat elliptical, although not perfectly so, and hints at a possible disk component. There appears to be some asymmetry in the outer regions suggesting minor gravitational disturbances.
