The galaxy presents a relatively smooth and featureless morphology. Its overall shape is elliptical, elongated with a slight flattening. The central region appears to be a bright, concentrated spheroid. The light distribution appears to follow a gradual decrease in intensity from the core outwards. There is subtle evidence of a disc structure within the galaxy, primarily in the form of the blue emission surrounding the bulge region. There is no apparent spiral arm structure. There is a possible minor disturbance that looks to be merging with the galaxy, though it is not clear. Overall, the appearance of this galaxy suggests that it is a relatively evolved and undisturbed system.
