The galaxy presents a generally smooth and featureless appearance. Its morphology is predominantly elliptical, exhibiting a moderately rounded shape. The central region displays a bright, concentrated luminosity, suggesting a high density of stars. Moving outwards from the core, the luminosity gradually decreases, fading into a diffuse halo. There appears to be a subtle colour gradient from the center to its edges. Some minor signs of tidal disturbances are suspected but there does not appear to be any major ongoing mergers.
