The galaxy presents an elliptical morphology, exhibiting a predominantly smooth, featureless structure. The central region displays a high concentration of light, indicative of a prominent galactic nucleus. Moving outwards from the core, the light intensity gradually diminishes, forming a diffuse halo. Subtle color variations are observed, transitioning from bluish hues near the central region to slightly redder tones in the outer edges, possibly reflecting differences in stellar populations. The overall appearance suggests a relatively evolved system with a moderate rate of star formation. There is no evidence of significant spiral arms or major distortions, although there may be signs of minor disturbances in the outskirts. It has a somewhat rounded shape, with no apparent interaction or merger activity.
