The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a prominent central bulge that appears yellowish-white, indicative of an older stellar population. Fainter, bluer light extends outwards from the core, suggesting some ongoing or recent star formation in the surrounding regions, though at a low rate. The overall shape is elongated, appearing cigar-shaped rather than perfectly spherical. There are no obvious signs of major disturbances such as tidal tails or close companions suggesting recent or ongoing major mergers, but there may be some minor irregularity. The galaxy is likely a mature system with a dominant old stellar population and a supermassive black hole in its center.
