The galaxy presents an overall elliptical morphology, elongated in shape. The central region exhibits a bright, concentrated core that fades gradually into the outer regions. The light distribution is relatively smooth, with no obvious spiral arm structures or prominent dust lanes visible. There is a suggestion of a disk component with a slight color change as you move away from the central core to the outer edge of the disk, from more yellow to more blue. There is no apparent ongoing major merging activity, although there might be very minor tidal disturbances present in the outer halo. The galaxy exhibits a relatively quiescent star formation rate, with no obvious bright, young stellar populations. The overall color suggests a population of older stars.
