The galaxy appears as a somewhat concentrated distribution of light, with a slightly elongated morphology. There is an indication of a diffuse halo surrounding a brighter central region. The light is primarily yellowish-red, suggesting an older stellar population, although some bluer components are visible in the periphery, potentially indicating regions of recent star formation. There appear to be some mild disturbances to the primary form of this galaxy, which could be the result of a past interaction. Overall, the galaxy exhibits a generally smooth appearance.
