The galaxy appears as a single, relatively smooth object with a concentrated central bulge or core, showing a high degree of circularity. The galaxy appears to be a single object, and has no major signs of merging. Color gradients are subtle, suggesting an older stellar population in the core. There may be some active star formation present, but it is not a dominant feature of the galaxy. The overall color index indicates the stellar population is dominated by redder stars. The galaxy is quite massive, but not extremely so. The morphology suggests a transition object between early and late type galaxies, or a massive early type galaxy.

