The galaxy presents as a somewhat symmetrical, centrally concentrated object with a diffuse morphology. The primary light emission appears yellow, suggesting a population of older stars. There are subtle, slightly elongated features visible, although they lack distinct boundaries. These could indicate a disk structure, or minor disturbances possibly resulting from past interactions. There is a general lack of well-defined spiral arms or bar-like structures in the visible light, although some hints of asymmetrical light distributions can be seen upon closer inspection. The galaxy's edges are not sharply defined, but rather fade gradually into the background sky. The smooth appearance suggests that this is a relatively massive galaxy.
