The observed galaxy presents a generally elliptical morphology. The central region exhibits a bright, concentrated luminosity, indicating a significant stellar density, potentially a bulge. Moving outwards, there is a somewhat ill-defined disk-like structure, with a lower surface brightness compared to the central bulge. Subtle color variations are observable, with a blue tinge throughout most of the galaxy and hints of red concentrated in the outer edges, possibly due to varying stellar populations or dust distribution. Some areas display minor visual irregularities. Overall, the galaxy appears largely unperturbed.
