The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a centrally concentrated luminosity profile, with a bright, yellowish core that gradually fades into a diffuse outer halo. The isophotes are generally round to slightly elliptical. There is no readily apparent spiral arm structure or significant dust lane obscuration, suggesting a lack of ongoing major star formation. Subtle color gradients are observed, with the core appearing more yellow and the outer regions exhibiting hints of bluer hues. This could indicate older stellar populations dominating the core and relatively younger populations towards the periphery. No obvious signs of tidal interactions or major mergers are visible. The overall morphology suggests a relatively evolved system.
