The galaxy exhibits a generally smooth morphology, with a high degree of central concentration. Its overall shape appears elliptical, approaching circular. There is little to no apparent disk structure. The galaxy's color profile transitions from a yellowish-white core to a bluer periphery. No significant signs of major disturbances or ongoing mergers are immediately evident, though minor asymmetries are visible at the edge. The galaxy is estimated to be a substantial system, presumably with a considerable stellar mass. It also exhibits some on going star formation.
