The galaxy presents as a largely smooth, centrally concentrated object. The core exhibits a high degree of luminosity, suggesting a dense population of stars and potentially a supermassive black hole actively accreting material. The luminosity appears to decrease radially outward from the central bulge.

The overall shape appears primarily elliptical, approaching a circular form, with only slight deviations from perfect roundness. There is no clear evidence of spiral arm structures or a defined disk component.

No strong evidence of ongoing major mergers or tidal disturbances are visible. The galaxy appears relatively undisturbed, suggesting that it is a fairly relaxed system that is nearing the end of its life.
