The galaxy presents as a lenticular or early-type spiral with a smooth, concentrated bulge. There is a slight elongation evident, suggesting a possible disk component viewed at a moderate inclination. The light profile appears relatively smooth, with no prominent spiral arms or distinct features immediately obvious. The dominant color is a yellowish-white, indicative of a population of older stars with suppressed star formation. Overall, it seems like a relatively massive system with relatively little ongoing star formation. Based on its morphology and color, the galaxy seems to be in the process of, or recently finished, transitioning away from being a very active star-forming galaxy.
