The galaxy presents as a moderately bright, elliptical structure with a smooth, diffuse appearance. Its core exhibits a concentrated, yellowish-orange hue, indicative of an older stellar population. The outer regions fade gradually, displaying a slightly bluer tint compared to the core, which may suggest some degree of recent star formation within the extended disk. The overall shape is somewhat elongated, deviating from a perfect circle, but does not show any obvious signs of major disturbances or ongoing mergers. There may be very minor signs of disturbance, but mostly it looks like a single spheroid object with no companions nearby. 
