The galaxy presents as a centrally concentrated, ellipsoidal structure. Its core exhibits a bright, yellowish-orange hue, possibly indicative of an older stellar population dominating the nuclear region. The galaxy's overall color gradient transitions to a slightly bluer tone in the outer regions, suggesting the presence of younger, bluer stars in these areas, though the color difference is subtle. The morphological classification appears to be that of an elliptical galaxy or a lenticular galaxy viewed at an angle. There is a slight extension along a major axis, giving it a somewhat elongated appearance. No distinct spiral arms or prominent dust lanes are discernible in the image. There is no apparent signs of tidal disturbances or recent merger activity.
