The galaxy presents as a relatively smooth, elliptical-like structure with a bright central bulge. The core appears intensely luminous, suggesting a high concentration of stars. The galaxy exhibits a slight elongation. The outer regions fade into the background sky. There is a subtle color gradient observed, with the central bulge appearing yellower in comparison to the slightly bluer, more diffuse halo. No distinct spiral arm structure is visible, and there is no indication of ongoing major merger activity or tidal disturbances. Overall, the galaxy presents a quiescent and evolved morphology.
