This galaxy presents a largely smooth, elliptical morphology. The central region exhibits a relatively high surface brightness, appearing nearly spheroidal. Moving outward, the light gradually fades, but retains a fairly regular elliptical profile without prominent spiral arms or a distinct disk structure.

The color gradient appears subtle, with the central region displaying a slightly yellower hue in comparison to the outer regions which trend towards bluer tones. This could indicate a relatively older stellar population concentrated towards the core, with ongoing, albeit diminished, star formation activity present in the outer regions. 

There is a slight irregularity in the overall light distribution suggesting a possible tidal interaction or recent minor merger.
