The galaxy appears to be a relatively bright, isolated object with a dominant spheroidal component. The light distribution suggests a smooth morphology, largely lacking in prominent spiral arms or other disk-like features. Its shape is somewhere in between round and elliptical, with a slight elongation along one axis. There is no obvious evidence of a major merger event in its recent history, although some minor disturbances or interactions cannot be ruled out.

The overall color suggests a population of older stars, with a relatively low rate of on-going star formation. The galaxy appears to be reasonably massive.
