This galaxy exhibits a relatively smooth morphology. While not perfectly spherical, it tends towards an elliptical shape, and the light appears diffused. There is no clear disk structure visible.

The color profile indicates a population of older stars. The light emitted appears to be more luminous in redder wavelengths. A small fraction of light appears to be emitted from a younger, bluer population of stars, suggesting a low level of ongoing star formation. There is no clear evidence of recent or ongoing major merger events, although there seems to be some kind of disturbance in the galaxy, possibly a minor merger.
