The galaxy presents as a relatively smooth, centrally concentrated object with a slightly elongated morphology. The central region exhibits a bright, yellowish-white hue, suggesting a population of older stars. Surrounding the core is a more diffuse, bluish halo, potentially indicating regions of ongoing star formation or a population of younger, hotter stars. There is a subtle asymmetry in the outer regions, perhaps hinting at a minor interaction or past merger event, though no strong tidal features are evident. Overall, the galaxy appears to be a relatively quiescent system. The colors suggest moderate star formation activity.
