The galaxy presents as a relatively smooth, elliptical morphology, appearing more in-between in shape than perfectly round. The color gradient indicates an older stellar population. The central bulge is characterized by a yellow-white hue, suggesting a concentration of evolved stars. Moving outward from the core, a diffuse, blueish halo is observed, potentially indicating the presence of younger stars or ongoing, albeit subdued, star formation. There is no clear evidence of spiral arms or a distinct disk structure. No major signs of disturbance are evident, suggesting that this galaxy has not experienced a major merging event recently.
