The galaxy presents as a somewhat diffuse object. Its morphology is largely smooth, exhibiting a centrally concentrated luminosity profile. The galaxy appears to be a spheroid with a largely featureless disk, which seems to be viewed at or near face-on. There are some slight irregularities in the light distribution, which may be due to minor disturbances within the galaxy's structure. The overall color of the galaxy suggests a evolved stellar population, indicative of low ongoing star formation.
