The galaxy presents a largely smooth, elliptical morphology. It exhibits a high degree of central concentration, with a bright, well-defined nucleus. The color is predominantly yellow to orange, suggesting a relatively older stellar population and low star formation activity. There is no obvious evidence of spiral arms or a disk structure. The shape is close to circular with no strong elongations. There is no indication of any major mergers, or other interactions. The galaxy is likely a massive system.
