The galaxy appears as a relatively smooth, somewhat rounded object. There is a slightly brighter, concentrated core region that exhibits a yellowish hue. Surrounding the core, the galaxy displays a fainter, more diffuse halo-like structure. The overall color suggests a population of older stars, though some bluer tinges within the halo suggest the presence of some younger stellar populations. There is some evidence of minor structural asymmetry within the galaxy, with a slight extension or distortion visible on one side. This could be indicative of tidal interactions or past minor merger events. The galaxy does not present any strong spiral arm features or a prominent disk component.
