The galaxy presents a smooth, elliptical morphology. The light distribution appears concentrated towards the center, with a radial falloff in surface brightness. A prominent, relatively bright core is visible. The galaxy exhibits a color gradient, transitioning from a yellowish-white hue in the core region to a slightly bluer shade in the outer regions. There is little evidence of significant spiral arm structure or irregular features; the galaxy appears largely undisturbed. Minor asymmetry is present on the outer edges. The overall appearance suggests a relatively evolved system dominated by older stellar populations, although the bluer color in the outer regions could imply some ongoing or recent star formation activity.
