The galaxy presents an elliptical morphology with a high degree of central concentration. The core region exhibits a significantly brighter luminosity compared to its outer regions. The galaxy's overall color appears relatively red-shifted. The isophotes display a somewhat flattened shape, deviating slightly from a perfect circle. The overall appearance suggests a mature stellar population, possibly with ongoing, but relatively low, star formation activity. There is no clear evidence of spiral arms or a prominent disk structure. No major disturbances from galaxy mergers are obvious.
