The galaxy presents as a fairly regular, elliptical morphology. The light distribution is smooth and centrally concentrated with a high degree of symmetry and no apparent strong tidal features. The galaxy is elongated, but not extremely cigar-shaped. There is a gradual decrease in luminosity from the core outwards, with no distinct spiral arms or disk structures visible.  The galaxy exhibits a slight color gradient, transitioning from a more reddish hue in the central region to a bluer tint in the outer regions. This could indicate a mixture of older stellar populations in the center and more recent star formation occurring in the outer regions. The galaxy exhibits no signs of major mergers, but some minor distortions may be present. These could indicate that it is currently undergoing or has recently undergone minor interactions.
