This galaxy presents as a relatively smooth, elliptical-like structure. The core region exhibits a concentrated, bright yellowish-orange hue, suggesting a population of older stars and a potential accumulation of dust. The color appears to redden towards the core. The overall shape is generally rounded, without any prominent spiral arms or disk-like features immediately apparent. There is a subtle fading in intensity as you move from the core to the outer regions of the galaxy. The outer edges lack sharp definition. There's a slight asymmetry or possible minor disturbance observed in the halo, possibly suggestive of a weak tidal interaction or minor merger event in its past or present. No major disturbances or merger events are visible. There is a bluer color shift in the extreme outer regions.
