The galaxy appears to be a relatively smooth, round object, likely an elliptical galaxy or a lenticular galaxy seen face-on. The central region exhibits a high degree of luminosity, suggesting a concentrated stellar population or possible active galactic nucleus. Moving outwards from the center, the intensity of light decreases. There are no distinct spiral arms or bar structures visible. There are some slight irregular forms on its outer boundary. This may signify minor disturbances. The galaxy demonstrates a redder hue, indicative of an older stellar population. The overall morphology suggests a system that is in a relatively evolved state.
