This galaxy exhibits a disk-like morphology, observed nearly edge-on. A prominent central bulge is visible, appearing centrally concentrated and rounded. The disk component is relatively thin, with some suggestion of dust lanes or obscuration along the galactic plane. The overall color profile suggests a population of older stars, with a moderate degree of ongoing star formation indicated by subtle variations in color. There does not seem to be a presence of any major mergers or interactions with any other galaxies, however a slight disturbance may be present. The smoothness in structure dominates.
