The galaxy presents a generally smooth, elliptical morphology. Its light profile appears concentrated towards the center, suggesting a prominent bulge component. The color distribution indicates a predominantly older stellar population, particularly within the central region which exhibits a yellowish hue. Fainter, bluer regions are subtly present in a diffuse disk component, indicative of possible ongoing, though low-level, star formation activity. There is no apparent major disruption in the galaxy's structure, but there are hints of minor distortions within the disk. The overall shape is roughly in between round and elongated.
