The galaxy presents a largely smooth, elliptical appearance. The central region exhibits a bright, concentrated luminosity, indicative of a significant stellar population. There is a slight elongation visible, deviating from a perfectly circular shape. A subtle color gradient is observed, transitioning from a yellower core to slightly redder outer regions, which potentially signifies variations in stellar age or metallicity. Furthermore, there may be some merging or minor disturbances happening in this galaxy.
