The galaxy appears as a relatively compact, elliptical-like structure. It exhibits a smooth, centrally concentrated morphology with a slight elongation along one axis, suggesting a possible transition state between elliptical and lenticular. The color profile indicates a dominant older stellar population, exhibiting a yellowish-gold hue, with some suggestions of bluer light on the edges indicating younger stars but at a very minimal presence. No obvious spiral arms or dust lanes are visible, consistent with a galaxy where star formation has largely ceased. The overall symmetry suggests that the galaxy is relatively undisturbed, showing no obvious signs of recent major mergers or tidal interactions. The galaxy presents a notable, but not exceptionally, high mass. Its current star formation rate is quite low.
