The galaxy appears as a somewhat diffuse object with a centrally concentrated luminosity profile. The overall color is a relatively neutral hue, suggesting an intermediate stellar population. There are hints of a disklike structure, but the galaxy is not highly flattened or strongly spiral in nature. Faint, irregular features are present around the central region, which could be interpreted as minor disturbances. There is no single dominant nucleus; the light is distributed in a relatively smooth manner, though there are irregular structures in the center, which suggests that there are regions of active star formation.
