The galaxy presents as a smooth, centrally concentrated object with a somewhat elliptical morphology. There is a distinct central bulge region that is brighter and more concentrated than the outer regions. The color of the galaxy appears to be generally redder, particularly within the central region, suggesting an older stellar population and a lower rate of ongoing star formation. There are no readily apparent spiral arm structures or prominent dust lanes visible in this image. The galaxy appears relatively undisturbed, without significant tidal features or signs of a recent major merger event. There are subtle indications of some extended, faint light surrounding the main body of the galaxy, which may be a stellar halo.
