The galaxy presents a generally smooth morphology. The light is centrally concentrated, appearing more luminous towards the galactic nucleus. The shape is roughly circular, with a degree of ellipticity, but not highly elongated. There is a faint, diffuse halo surrounding the central region, which could be indicative of an older stellar population. There may be some faint features, perhaps indicating the presence of a disk; however, these features are not pronounced. There is no visually apparent interaction with any other galaxy. It appears to be a relatively isolated system, which might have undergone a minor disturbance sometime in the past. Color analysis indicates a higher concentration of redder light, which suggests a larger presence of older stars. There is a faint yellow hue present in the center of the galaxy, perhaps indicative of a burst of star formation, but the galaxy is not as active as a spiral galaxy with many blue stars.
