The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a high degree of luminosity, appearing almost uniformly bright. The light gradually diffuses outward, creating a relatively even gradient towards the galactic periphery. There is a slight elongation, but overall, the galaxy maintains a consistently rounded shape. Subtle color variations are observed; bluer tones are present toward the central region, while the outer edges appear slightly redder. This may be due to different stellar populations. Indications of disturbances are minimal, suggesting a stable system.
