The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a concentrated, bright, yellowish-white core, suggesting an older stellar population. Fainter, somewhat diffuse, greenish regions are present in the outer areas. These suggest the possibility of some ongoing, though limited, star formation. There is no discernable disk structure or spiral arm morphology present. There is also no evidence of any strong tidal features or obvious signs of mergers. The overall shape is more rounded than elongated.
