The galaxy presents an elongated, cigar-shaped morphology, potentially indicative of an edge-on spiral or an elliptical galaxy. The light distribution is relatively smooth, but there are hints of a disk-like structure. There is a central bulge that is apparent. The galaxy is primarily composed of older stars. There is some irregular light distribution in areas around the center bulge, but it does not indicate major galactic disturbances or mergers. There is indication of some very low level star formation. The overall color suggests a modest amount of dust obscuration.
