The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. The morphology suggests a classification towards the earlier types, potentially an E or S0 galaxy. There is a slight elongation visible, implying it is not perfectly spherical but rather somewhat flattened. The color appears predominantly blue, suggesting a population of younger, hotter stars, though this could also be influenced by the presence of ionized gas. The overall structure lacks distinct features such as spiral arms or prominent dust lanes, further supporting the smooth classification. There may be some subtle disturbances, but the galaxy mainly appears isolated.
