The galaxy appears as a centrally concentrated elliptical object with a smooth, diffuse morphology. The light profile shows a radial decrease in intensity from the core outwards. There is a noticeable color gradient, exhibiting a yellowish-orange hue in the central region, which transitions to a bluer tint in the outer regions. This suggests a possible mix of older stellar populations towards the core and younger populations in the outer regions, even though no distinct spiral arms or disk-like features are visible. The overall shape is slightly elongated, and no significant tidal disturbances or signs of ongoing mergers are apparent. 
