The galaxy presents an elliptical morphology, appearing largely smooth in texture, with only minor disturbances. It is elongated in shape and has an apparent color gradient, transitioning from a bright, reddish-yellow core to a fainter, slightly bluer periphery. This color distribution suggests a population of older stars concentrated in the core, with younger, bluer stars possibly existing in the galaxy's outer regions, though current rates of star formation are likely low. There is no readily apparent spiral arm structure. The general appearance implies that the galaxy is relatively evolved.
