The galaxy presents as a relatively smooth and centrally concentrated object. It exhibits an overall elliptical morphology, lacking any apparent spiral arm structure or a well-defined disk. The color profile suggests a dominant population of older stars, with a central yellowish hue transitioning to a redder, less luminous halo region. There are no discernible signs of active star formation or significant dust lanes within the galaxy's visible structure. The galaxy appears to be relatively undisturbed, without any major distortions or tidal features that would indicate a recent merger event.
