The galaxy presents a largely smooth and elliptical morphology. It exhibits a concentrated central bulge which diffuses outwards. The color profile suggests a moderate population of older stars, giving it a yellowish-white hue in the central regions. There's a slight hint of bluer tones in the outer regions, suggesting the presence of a small population of younger, hotter stars, although star formation appears to be relatively quiescent overall. No spiral arm structure or significant dust lanes are readily apparent. There are no signs of any major ongoing merger events or tidal disturbances, with only very minor asymmetries visible which could indicate a slight disturbance. The galaxy appears to be relatively isolated in the field. 
