The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a high surface brightness, appearing nearly spherical. The radial intensity profile appears to decrease smoothly from the center, transitioning into a diffuse halo. There is a noticeable absence of distinct spiral arm structures or significant dust lanes. Hints of blue color are observed in the core of the galaxy, which could indicate some ongoing star formation. There is no clear evidence of tidal tails or morphological disturbances to suggest recent or ongoing merger activity. Overall, the galaxy appears to be an early-type system with a quiescent star formation rate.
