The galaxy presents as a relatively smooth, elliptical morphology. Its color profile exhibits a central concentration of yellowish light, which fades into a bluish hue towards the outer edges. The overall shape appears somewhat rounded. There is no obvious indication of a spiral arm structure or a central bar. Faint hints of minor disturbances might be present in the outer regions, but the dominant impression is that of a relaxed system. Based on the color indices, the stellar population appears to be relatively old on average. Active star formation seems limited to moderate levels. There is no sign of a major ongoing merger event.
