This galaxy presents an overall elliptical morphology, appearing elongated in shape. The central bulge region exhibits a bright, concentrated luminosity, indicative of a high stellar density. Moving outward from the core, a diffuse halo or disk-like structure is observed. The colour gradient suggests a change in stellar populations with bluer tones in the outer regions, which potentially points to ongoing or recent star formation. No distinct spiral arm structures are visible. There is a slight asymmetry with a slight tidal disturbance on one side, perhaps indicating a minor interaction, though this appears to be a relaxed system overall. 
