The galaxy presents as an elliptical morphology. The light distribution appears relatively smooth, suggesting an older stellar population. The galaxy displays a concentrated central bulge which graduates into a diffuse halo. The observed color appears to be more heavily weighted in the redder part of the spectrum, but also displays some evidence of blue light. There are no readily apparent spiral arm structures or dust lanes. No significant tidal distortions or features indicative of a major merger are visible, although there is a hint of minor disturbances. The galaxy exhibits an intermediate axial ratio, neither perfectly spherical nor highly flattened.
