The galaxy presents as a centrally concentrated object, with a dominant, smooth bulge-like structure exhibiting a yellowish-orange hue. The radial light profile appears to decrease steadily from the center outwards, suggesting a relatively old stellar population in the core. There's evidence of a faint, diffuse disk component extending from the central bulge. The outer regions of the galaxy show slightly bluer colors, which may indicate ongoing or recent star formation in these areas, although it is not very prominent. There seems to be a disturbance off to the upper right side of the galaxy. The overall shape of the galaxy is somewhat elliptical, but shows signs of a more irregular morphology.
