The galaxy appears as a single, relatively smooth concentration of light. The central region exhibits a reddish hue, suggesting an older stellar population or dust obscuration. Surrounding this central region, there's a more diffuse halo of greenish light, possibly indicating a population of younger, hotter stars. There's no readily apparent spiral structure or distinct features such as a bar or tidal tails. The overall shape is roughly elliptical or spheroidal, with a high degree of central concentration. There's no visual evidence of a major ongoing merger or significant disturbances in the galaxy's structure.
