The galaxy presents a generally smooth morphology, suggesting an elliptical or lenticular classification. It exhibits a centrally concentrated luminosity profile, with a bright, yellowish core that gradually fades towards the outer regions. There is evidence of some disk like structure, along with low amounts of irregular structure. Subtle color gradients are observable, with slightly redder tones appearing in the inner regions with bluer tones in the outer regions. The galaxy displays an overall roundness, with a minor extension along one axis, ruling out a highly elongated or cigar-shaped structure. There is no prominent evidence of ongoing major merger activity, although subtle signs of minor disturbances or tidal features cannot be entirely ruled out.
