The galaxy presents a somewhat elliptical morphology, with a centrally concentrated bulge. The bulge exhibits a yellowish-white hue, indicative of an older stellar population. The disk component appears fainter and exhibits a bluer color gradient moving outward from the central bulge. The smooth, relatively uniform appearance of the galaxy indicates that it is likely a disk galaxy with a dominating bulge. There is a slight hint of possible disturbance in the overall structure but more information is necessary to be sure. The object seems to be relatively massive with some small amount of star formation.