The galaxy appears as a slightly elliptical, concentrated light source. The core exhibits a strong, golden hue, suggesting a population of older stars. Adjacent to this central region, there is a fainter, less defined area with a hint of greenish-blue color, which might indicate ongoing or recent star formation. This less-defined area seems to be merging with a nearby object. The galaxy lacks a clear spiral arm structure, indicating either a smooth morphology or the early stages of a merger event. There are minor disturbances visible within the galaxy. The outer regions of the galaxy fade gradually, indicating a diffuse halo.
