The galaxy appears as a centrally concentrated, roughly elliptical object. The central region exhibits a bright, yellowish-white hue, possibly indicating an older stellar population. There is a subtle color gradient moving outward from the core, transitioning to a slightly redder and dimmer halo. The galaxy is dominated by a smooth, featureless morphology, lacking any prominent spiral arms or significant dust lanes. There is a slight elongation in the galaxy's shape, classifying it as more 'in between' in roundness than purely spherical. The overall structure suggests a relatively evolved system, possibly undergoing little to no major merging activity and with a low rate of star formation. No significant tidal features or morphological disturbances are immediately apparent.
