The galaxy exhibits an elliptical morphology, appearing largely smooth and featureless. There is a centrally concentrated bulge that dominates the galaxy's overall structure. The light distribution suggests a relatively uniform stellar population, with a gradual decline in intensity from the core outwards. There are hints of a subtle color gradient, with the central regions potentially exhibiting a slightly yellower or redder hue. The shape of the galaxy is nearly circular, exhibiting only slight elongation. There is no clear evidence of spiral arm structure or a prominent disk component. Overall, the galaxy presents as a relatively undisturbed and evolved system.
