The galaxy presents a generally smooth, elliptical appearance. The central region exhibits a significantly higher surface brightness, appearing nearly circular. A subtle color gradient is observed, with the core exhibiting a yellowish-white hue, transitioning to a bluer tint in the outer regions. The shape shows a slight elongation, the major axis is discernable from the minor axis. No distinct spiral arms or prominent dust lanes are visible, suggesting a relatively quiescent morphology. There is no apparent evidence of ongoing major merging events or significant tidal disturbances, although there are subtle indications of minor disturbances. The light distribution suggests a Sersic profile, with a moderate concentration of light in the core. The relative flux in the redder bands seems higher, indicating a possibly older stellar population.
