The galaxy presents a largely smooth morphology. It has a near-spherical appearance, showing a relatively high degree of central concentration. The color profile is predominantly yellowish-orange, indicative of an older stellar population with relatively lower levels of ongoing star formation. There is a subtle hint of bluer tones in its outer regions, possibly suggesting the presence of younger, hotter stars, albeit at a lower overall rate. No prominent features such as spiral arms or a distinct galactic bar are discernible, implying the object is an elliptical galaxy or a lenticular galaxy seen face-on. There is no apparent ongoing major merger, or signs of significant tidal disruption.
