The galaxy presents an overall elliptical morphology, appearing largely smooth and centrally concentrated. A bright, condensed core region is visible, exhibiting a yellowish-orange hue, suggesting a population of older stars. The intensity of the light gradually diminishes outward from the core, transitioning into a fainter halo. There are no apparent spiral arms or significant dust lanes discernible. The overall form is more akin to an elliptical galaxy than a spiral one, with little indication of ongoing major star formation. There may be a slight ellipticity to the overall shape, but it is mostly uniform and without major disturbances from mergers, suggesting a relatively relaxed dynamical state.
