The galaxy appears to be a relatively smooth and centrally concentrated system. It displays a moderate degree of ellipticity, appearing somewhat flattened rather than perfectly spherical. The central region exhibits a yellowish hue, suggesting an older stellar population dominates the core. A faint, bluer halo surrounds the central bulge, indicating the presence of some younger stars and possibly ongoing star formation in the outer regions. There are no prominent spiral arms or obvious signs of a recent major merger event. The galaxy appears relatively isolated, with no close companions or significant tidal disturbances visible.
